The galaxy presents as an elongated, elliptical shape with a smooth, diffused light distribution. The central region exhibits a higher concentration of luminosity, appearing more yellowish-orange in color, indicative of an older stellar population. Moving outward from the core, the color transitions to a fainter, slightly bluer hue, suggestive of a younger stellar population. There is no clear evidence of spiral arms or a distinct galactic disk, pointing towards a spheroid-dominated morphology. Overall, the galaxy's structure appears relatively undisturbed with no major tidal features or evidence of ongoing merging activity visible in this image.
