The galaxy presents as a generally smooth, elliptical-like structure. There is a bright, concentrated central bulge that appears yellowish. Extending outwards from the bulge is a more diffuse region with fainter, bluer tinges. There is a slight asymmetry in the outer regions of the galaxy, suggesting a possible disturbance or interaction. The object is predominantly smooth in appearance with some subtle features, potentially a faint disk-like component or tidal debris. There is no clear evidence of a major ongoing merger, but some minor disturbances can be detected from its shape. The concentration of light towards the center is very noticeable. The galaxy's overall colour profile suggests a mix of stellar populations, with an older population dominating the central bulge and a younger, possibly star-forming population present in the outer regions. The galaxy is neither perfectly round nor highly elongated but sits in-between, appearing slightly ellipsoidal.
