The galaxy appears as a single, fairly smooth, and concentrated object. It exhibits a generally round morphology, with little indication of a disk-like structure or significant tidal disturbances. The light profile of the galaxy suggests a relatively even distribution, with a central concentration that diminishes gradually toward the outer regions. The dominant color is a yellowish hue, which may indicate an older stellar population. There is minimal evidence of active star formation within the galaxy. Overall, it appears to be a fairly evolved system.
