This galaxy presents as a system with a dominant central body and some possible indications of interaction or tidal features. The primary galaxy exhibits a relatively smooth, elliptical morphology. There is a concentrated nucleus with a gradual decrease in luminosity outward. The central region appears yellow-white suggesting an older stellar population. The outer regions display a bluer hue which could indicate the presence of younger stars. The overall structure is primarily spheroidal with a slight elongation. There is a notable asymmetry in the light distribution, suggesting that it is not a perfect elliptical. A faint plume or tidal tail is visible on one side of the galaxy, hinting at a past or ongoing interaction. This disturbance appears relatively minor but could be the result of a merger with a dwarf galaxy or a close encounter with another system.
