The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The overall shape is relatively round, lacking any significant elongation or bar structures. There is little evidence of spiral arms or distinct features indicative of ongoing star formation. The galaxy displays a subtle color gradient, appearing slightly bluer towards the center, suggestive of a potentially younger stellar population or weak active galactic nucleus activity in the core region. There are no obvious signs of major mergers or tidal disturbances, but a subtle asymmetry in the outer halo could indicate a minor interaction or accretion event in the past.
