The galaxy presents as a relatively smooth object with a centrally concentrated luminosity profile. It appears elliptical in shape, exhibiting a high degree of roundness. There is a subtle color gradient, with the core appearing slightly more yellow/red than the outer regions, suggestive of an older stellar population in the nucleus. There is little evidence of spiral arms or distinct disk features. The galaxy displays no obvious signs of major mergers or tidal disturbances, but a very slight asymmetry is present, it may be indicative of a minor interaction or internal dynamics. The overall color suggests that the galaxy is a relatively evolved system, with moderate mass, currently experiencing low levels of star formation. The scale of the object indicates that it is a relatively small galaxy.
