The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge characterized by a yellowish hue, suggestive of an older stellar population. Surrounding the core is a fainter, diffuse halo with a slightly bluish tint, potentially indicating the presence of younger stars or ongoing star formation at a relatively low rate. The galaxy does not display any obvious spiral arms or bar structures. There is no visual indication of any major ongoing merging activity or significant tidal disturbances. The galaxy appears moderately luminous with a relatively compact size. Its shape is best described as being in between round and cigar-shaped.
