The galaxy presents a largely smooth and rounded morphology. There is a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. The outer regions appear more diffuse, fading into the background sky. No prominent spiral arms or distinct disk features are readily discernible in the image. There is no obvious visual evidence of ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated, lacking close companion galaxies or significant signs of interaction. Based on its color and morphology, the galaxy could be classified as an elliptical or S0 type galaxy.
