The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. The overall shape is more lenticular than spherical, appearing somewhat flattened. The color profile suggests an older stellar population, with a yellow-red hue dominating, indicative of reduced recent star formation. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. The galaxy seems to be largely undisturbed, showing no obvious signs of a major merger event, although there is the suggestion of a very minor disturbance in the morphology. The overall appearance indicates a galaxy transitioning towards a quiescent state, with diminished star-forming activity.
