The galaxy presents a generally smooth morphology, appearing largely spheroidal. There is little evidence of prominent spiral arm structure or a distinct disk. It appears relatively round in shape. The galaxy's light is concentrated towards the center, indicating a possible central bulge. There is a subtle color gradient, with the core exhibiting a slightly yellowish hue, possibly indicative of an older stellar population. The outer regions appear fainter with no easily distinguishable features. There are no visible signs of a major ongoing merger, although there might be a minor disturbance or interaction in the galaxy's vicinity or a faint tidal tail that is not distinctly visible. The galaxy exhibits a moderate degree of luminosity.
