The galaxy presents as a relatively smooth, elliptical-like structure. There is a distinct, brighter core that transitions outward to a diffuse halo. The overall shape appears to be somewhat elongated rather than perfectly spherical, suggesting a possible deviation from a pure elliptical morphology. There seems to be a second smaller galaxy nearby that may be merging, with noticeable disruptions in the main galaxy's morphology possibly indicating interactions. Star formation appears moderate across the system. The galaxy exhibits a generally red color, indicative of an older stellar population.
