The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in surface brightness moving outwards from the core. The core is a diffuse white/pink, surrounded by a greenish-yellow halo, with low contrast, suggestive of an older stellar population and a lack of significant ongoing star formation. There are no discernible spiral arms or dust lanes visible in this image. The galaxy appears relatively undisturbed, lacking any strong tidal features or asymmetries that would suggest recent merger activity or strong gravitational interactions. It is characterized by a high degree of roundness. The slight color variation, specifically the redder core, suggests a concentration of older, redder stars in the galaxy's center.
