The galaxy presents as a well-defined, elliptical morphology. Its light profile is centrally concentrated, with the highest surface brightness observed toward the galactic nucleus. The isophotes appear relatively smooth, indicating a lack of significant dust lanes or spiral arm structures. The galaxy exhibits a gradual decrease in surface brightness from the core outward to the edges. The overall color appears to be yellowish or golden, suggestive of an older stellar population. The absence of distinct blue regions implies that the galaxy may have a relatively low star formation rate. While the galaxy exhibits an oval shape, there appears to be no significant asymmetry or tidal features that would indicate recent or ongoing merger activity, although some minor disturbances cannot be ruled out based on the faintness of the outer regions. It does not appear perfectly round but instead exhibits a shape somewhere between round and cigar-shaped.
