The galaxy appears as a relatively compact, elliptical structure. It exhibits a smooth light distribution with no apparent spiral arms or bar features. The light profile is centrally concentrated, decreasing outwards with a noticeable falloff. The galaxy's overall shape appears quite rounded, although there is some potential asymmetry in the light distribution which could suggest a mild interaction or past merger event. There is an indication of some disturbed morphology, it's not perfectly symmetric. The galaxy exhibits a blueish hue in its center, this could indicate recent or current star formation. 
