This galaxy presents as two distinct components, suggesting a possible interaction or merger event. The primary component exhibits a relatively smooth, elliptical morphology, characterized by a bright central bulge. The bulge demonstrates a color gradient, appearing more yellow toward the center and transitioning to a slightly bluer hue outwards.

A secondary, elongated structure extends from the primary component, displaying a more diffuse and irregular shape. This feature exhibits a significantly bluer color profile compared to the primary bulge, indicative of a younger stellar population or ongoing star formation. The connection between the two components is noticeable, and the observed morphology indicates a possible tidal tail or stream resulting from a gravitational interaction.

Overall, the galaxy's morphology deviates from a purely elliptical or spiral classification, suggesting that it might be a galaxy undergoing a merger. Evidence exists for a possible minor disturbance in the galaxy's morphological integrity, though definitive confirmation would require further spectroscopic or imaging observations.
