The galaxy presents as a moderately luminous elliptical morphology. The light is dominated by a smooth, centrally concentrated bulge. There is little to no evidence of spiral arm structure or a distinct disk component; the transition from the bulge to the outer regions appears gradual. The color of the bulge is yellowish-white, suggestive of an older stellar population with a relatively low rate of ongoing star formation. The galaxy exhibits a slight elongation, with an apparent axial ratio indicating it is neither perfectly spherical nor highly flattened. There are no obvious signs of tidal disturbances or major mergers, although some subtle asymmetry in the outer halo might hint at minor interaction history. Overall, the galaxy appears to be a relatively quiescent elliptical system, likely composed of predominantly old stars and with low current star formation activity.
