The galaxy presents as a generally smooth, elliptical structure with a concentrated central bulge. The color gradient indicates a population of older stars, trending toward a redder hue in the core and fading into a diffuse yellowish halo. No spiral arms or disk-like features are discernible. The overall morphology suggests a relatively evolved system, potentially with low recent star formation activity. There's no obvious evidence of on-going mergers or tidal disturbances from nearby companions. The galaxy appears fairly isolated and relaxed in its current state.
