The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology without prominent spiral arms or a distinct disk. It possesses a concentrated central bulge that is bright in yellow, suggesting a high density of older stars. The galaxy is elongated, with a slight flattening visible. The outer regions of the galaxy appear fainter and more diffuse, transitioning gradually into the background sky. The light distribution shows a centrally peaked profile, consistent with a high Sersic index, with an estimated half-light radius of around 6 kpc. The color indices indicate a redder overall color, which implies a stellar population dominated by older, redder stars and minimal ongoing star formation. This is further supported by the low specific star formation rate, which suggests it is likely a quiescent or passively evolving system. There is very little evidence of dust lanes or other irregular features. The galaxy does not appear to be undergoing any major merger activity.