The galaxy appears as a moderately bright, elliptical object with a smooth, diffuse profile. It exhibits a generally rounded morphology, with no discernible spiral arms or distinct disk structures. The light distribution suggests a relatively homogeneous stellar population, with a concentration of intensity towards the central region, typical of elliptical galaxies. There is a slight color gradient across the galaxy, with a subtle reddening towards the core, which could indicate a higher concentration of older, redder stars in that region. No obvious signs of recent major merger activity or strong tidal disturbances are apparent, although a subtle asymmetry might suggest a past minor interaction. The overall appearance suggests a relatively evolved system, likely with a significant population of older stars and a moderate mass.
