The galaxy presents as a relatively smooth, single structure. It exhibits an elliptical morphology, with the central region displaying a high degree of symmetry and a gradual decrease in luminosity outward. The galaxy is characterized by a generally homogeneous color profile. A slight elongation is observed, deviating from a perfectly circular shape. There is no apparent spiral structure, distinct dust lanes, or prominent star-forming regions visible. The overall appearance suggests a relatively quiescent system, possibly a mature galaxy with limited ongoing star formation. Evidence may suggest a past, small merger event.
