The galaxy presents as a slightly elongated, lenticular structure. A bright, concentrated central bulge dominates the morphology, exhibiting a smooth, featureless appearance. Moving outward from the core, the galactic disk appears less defined. There may be slight disturbances in the outer regions, but the overall impression is of a galaxy undergoing only minor, if any, gravitational interaction with a neighbor. The overall color profile indicates a population of older stars, with only faint indications of active star formation. A small degree of tidal debris or faint extensions could be present, but the faintness and subtle color changes suggest a quiescent galaxy in a relatively isolated environment.
