The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology with a distinct bulge component. A slight elongation is observed, but it does not appear strongly barred or cigar-shaped. Some asymmetric features can be seen extending from the central bulge, likely indicating either tidal disturbances from a past interaction or early stages of spiral arm formation. The galaxy's color profile suggests a mix of stellar populations, with a redder hue in the central region and a slightly bluer tint in the outer disk. A potential merging event cannot be fully excluded given the disturbances. Overall, the galaxy is likely a transition object, possessing characteristics of both elliptical and spiral galaxies.
