The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, appearing bright and nearly spherical. Moving outward from the core, the light gradually diminishes, transitioning into an elongated shape. The observed color suggests a population of older stars, with a yellowish-red hue dominating. No distinct spiral arm structures or prominent dust lanes are discernible. There is no evidence of a recent major merger, though subtle asymmetry in the outer regions could suggest minor tidal interactions or past disturbances. The galaxy's overall appearance points towards a relatively evolved system with a quiescent star formation rate.
