The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest in its core, with light gradually diminishing outwards. The core region displays a yellowish hue, possibly indicative of an older stellar population. Moving outwards from the core, the galaxy transitions to a bluer color in the outer regions, which might suggest the presence of a younger stellar population or ongoing star formation. There appears to be a slight asymmetry in the outer regions, though not indicative of a major ongoing merger. There is no distinct disk structure visible. The galaxy appears relatively undisturbed.