The galaxy presents as a relatively smooth, centrally concentrated object. There is a lack of defined spiral arms or a prominent disk structure, suggesting it may be an elliptical or lenticular galaxy. The light distribution appears centrally condensed with a gradual decrease in intensity outwards, contributing to a fairly round overall shape. The core region of the galaxy shows a brighter, more intense emission. There is no visual evidence of tidal tails, major disturbances, or ongoing mergers. The color appears to be fairly uniform across the galaxy, leaning towards slightly redder hues. The estimated size is relatively compact.
