The galaxy presents as a generally smooth and rounded object. It exhibits a concentrated central bulge or core that is significantly brighter and more yellow than its surrounding regions. This suggests an older stellar population dominates the core, with a dearth of ongoing star formation.

The outer regions of the galaxy appear less concentrated and show a bluer hue, although the color is still relatively muted, this may indicate the presence of younger, hotter stars, but likely at a very low rate. There is no clear evidence of spiral arm structure, bars, or significant dust lanes. The galaxy appears largely undisturbed, exhibiting no obvious signs of major mergers or tidal interactions. Its morphology is consistent with an elliptical galaxy. The estimated size is approximately 5 kpc in radius.

