The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears largely spheroidal, suggesting an elliptical morphology. It exhibits a prominent bulge region that dominates the overall luminosity. Moving outwards from the center, the galaxy fades into a fainter, more diffuse halo. There is a slight elongation, but overall the galaxy appears quite round. No distinct spiral arm structures are discernible. The galaxy's color is generally yellowish, potentially indicating an older stellar population with limited ongoing star formation. There is a possible hint of a very faint, slightly bluer disk component, but it is not well-defined. There is no evidence of strong tidal features or ongoing major mergers. The slight asymmetry in the outer regions may suggest past minor interactions or accretion events.
