The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge exhibiting a yellow-white hue, suggestive of an older stellar population. The overall shape is somewhere between round and elongated. There is a faint, diffuse halo extending beyond the central region. A subtle disturbance or asymmetry is observed in the halo region. There may have been a past minor merger event or tidal interaction. The color gradient suggests a decline in star formation activity from the core outwards. The galaxy exhibits an absolute magnitude of -20.56 in the R band, suggesting a somewhat less luminous galaxy.
