The galaxy presents an elliptical morphology, exhibiting a generally smooth appearance with no readily apparent spiral arm structures. The light distribution suggests a centrally concentrated bulge, which is likely an old, redder stellar population. The outer regions of the galaxy appear less luminous and more diffuse, fading gradually into the background sky. The orientation of the galaxy is neither face-on nor edge-on, showing an intermediate inclination. A slight asymmetry in the overall shape may indicate the presence of minor disturbances, possibly due to a past merger event. Overall, this galaxy appears to be an evolved system, consistent with a classification of an early-type galaxy.
