The galaxy appears as an elliptical or lenticular-like structure with a smooth, concentrated central bulge. The light distribution indicates a centrally-peaked luminosity profile, typical of early-type galaxies. There is a slight elongation or flattening visible in the galaxy's shape. A faint, diffuse halo or disk component is also present. There is no clear evidence of strong spiral arms, prominent dust lanes, or irregular features associated with recent major merger events. There appears to be a lack of recent star formation. A possible tidal tail is present.
