The galaxy presents a primarily elliptical morphology. It appears relatively smooth in structure, exhibiting a concentrated central bulge with a gradual decrease in luminosity outward. There is a subtle flattening, suggesting it may be an elliptical galaxy of type E4-E5. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating this region. The outer regions display a slightly bluer tint, hinting at the possibility of ongoing, albeit subdued, star formation in the galactic disk. There does not appear to be any significant tidal disruption or ongoing major merging activity in the galaxy. It is likely a relatively isolated system undergoing normal galactic evolution.
