The galaxy presents a generally smooth, elliptical morphology. It appears to be elongated, displaying a cigar-shaped profile rather than a perfectly circular one. A concentrated, bright central bulge is evident, suggesting a significant population of older stars. The galaxy exhibits a gradual decrease in luminosity from the core to the outer regions. No distinct spiral arm structures are discernible, and there is no evidence of major mergers or tidal disturbances. The galaxy shows a color gradient from a yellowish central region to bluer, less intense outer regions. The lack of obvious dust lanes further contributes to its smooth overall appearance.
