The object appears as a concentrated elliptical galaxy displaying a smooth morphology with minimal observable substructure. The galaxy exhibits a bright central bulge that gradually diminishes in luminosity towards the outer regions, suggesting a high degree of radial symmetry. There is no obvious presence of spiral arms or a pronounced disk structure. Some light appears to be from minor disturbances. The color gradient appears to be a redder hue towards the core, with a color shift blueish hues in the outer regions. The overall color indicates that this galaxy is likely composed of an older stellar population, although bluer light may indicate some younger star formation. No evidence of tidal tails, strong distortions, or a clear merger companion.
