The galaxy presents an elliptical morphology, appearing smooth and somewhat elongated, with an aspect ratio suggesting a moderate degree of flattening. The central region exhibits a higher surface brightness, indicative of a prominent bulge. A gradual decrease in luminosity is observed moving outward from the core, with no distinct spiral arm structures or prominent dust lanes visible. The color profile suggests a relatively evolved stellar population, with a yellowish-white hue in the central region that transitions to a slightly bluer tint in the outer regions, consistent with ongoing, but potentially subdued, star formation activity. There is no strong visual evidence of any major merging events or significant tidal disturbances, though subtle asymmetries cannot be ruled out. The overall appearance suggests an intermediate to high mass system with a relatively quiescent star formation rate.
