The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be elliptical, exhibiting a gradual decrease in surface brightness from a bright, yellowish core outwards. While mostly smooth, there are faint indications of some substructure or features.

The color profile suggests an older stellar population, with a dominant yellow hue indicating a lack of significant recent star formation. However, there may be subtle hints of bluer regions, especially in the outer areas, suggesting a small amount of ongoing or recent star formation activity there.

The overall shape is somewhat elongated but fairly close to round, and there are no obvious signs of tidal tails, distortions, or interactions that would suggest a recent major merger event. There might be a minor disturbance or a faint, diffuse plume on one side, but more data would be necessary to confirm this. 
