The galaxy presents a flattened, elliptical morphology, with a major axis that appears to be oriented horizontally within the image frame. The central region exhibits a high degree of luminosity, with a smooth, concentrated distribution of light. The color of this central bulge is distinctly yellowish, potentially indicative of an older stellar population. Extending outward from the bulge, a fainter, more diffuse disk is observed. Hints of bluer light are present within the disk, most notably along the lower border where a slight concentration of this blue light can be seen, suggesting regions of more recent star formation. Overall, the galaxy displays a relatively smooth appearance, with no obvious signs of major disruptions or ongoing mergers. There is a slight hint of minor tidal disturbance, but the dominant visual impression is that of a relatively undisturbed system with characteristics intermediate between a pure elliptical and a spiral galaxy. The concentration of light is highest toward the center, gradually diminishing outward in a smooth fashion. The axial ratio suggests a moderately inclined disk system viewed at a non-negligible angle to the line of sight.
