The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. The color profile suggests an older stellar population dominating the bulge, indicated by the yellowish hue. The outer regions of the galaxy display a fainter, bluer tint, potentially indicating the presence of some younger stars or ongoing star formation within a disk structure. The overall structure exhibits some signs of possible tidal disturbances or interactions, with asymmetries in the outer isophotes and faint extensions suggesting a minor merging event. The galaxy appears fairly massive, with a substantial contribution from older stars, while exhibiting a low star formation rate overall.
