The galaxy exhibits a smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure.  Its light profile appears centrally concentrated, with a gradual decrease in brightness towards the outer regions.  The color gradient suggests an older stellar population, with a yellowish hue dominating the galaxy's core.  The galaxy appears moderately flattened, with its semi-major axis displaying a clear elongation when compared to its semi-minor axis. There is no clear indication of ongoing major star formation, though there may be trace amounts occuring, as hinted by subtle variations in color. The overall structure suggests that this is a relatively undisturbed galaxy that has not undergone any major merging events recently.
