The galaxy appears as a centrally concentrated object with a roughly elliptical morphology. The central region exhibits a bright, smooth appearance, suggesting a substantial stellar population. Moving outwards from the center, a fainter, diffuse halo or disk-like structure is observed, exhibiting a bluer color compared to the core. This color gradient could indicate the presence of younger stars and ongoing star formation in the outer regions of the galaxy, though at a moderate or low rate. The overall smoothness of the galaxy's light distribution suggests it is likely a relatively evolved system, with minimal evidence of significant recent mergers or tidal disturbances. There is a slight elongation to the overall shape, tending toward a more cigar-shaped appearance.
