The galaxy presents as a diffuse, centrally concentrated object. It appears to be relatively smooth in texture, with a possible slight elongation, but lacks any distinct spiral arm structure. The color profile suggests a dominance of older stellar populations, indicated by its reddish-orange hue, particularly within the central bulge. The outer regions appear slightly bluer, perhaps indicative of more recent, albeit subdued, star formation activity in these areas. Overall, the morphology leans toward an elliptical or lenticular classification, though some disturbed structure is also visible. Some evidence of a possible merger or tidal interaction with a smaller companion object is indicated.
