The galaxy exhibits a predominantly smooth morphology, appearing elliptical in shape with a high degree of central concentration. The color profile is dominated by redder hues, suggestive of an older stellar population. A slight elongation is observed, though the axial ratio indicates a near-circular appearance. There is no obvious evidence of spiral arm structure or prominent dust lanes. The galaxy appears relatively undisturbed, lacking any signs of major mergers or tidal features. The overall impression is that of a relatively massive, quiescent galaxy with a low rate of star formation.
