The galaxy presents an elliptical morphology, displaying a centrally concentrated bulge with a smooth, diffuse halo extending outwards. The core region exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the core, the color gradient shifts towards a slightly bluer tint, suggesting the presence of more recent star formation in the outer regions of the galaxy. There are some indications of tidal disturbances with a lopsided structure to the left and above the central bulge. Faint wisps or extensions are observed, possibly due to gravitational interactions with a possible merging partner. The overall structure suggests a system undergoing or having recently undergone a significant interaction or merger event. The observed features indicate a complex interplay between older stellar populations, on-going star formation, and gravitational dynamics.
