The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical in shape. The radial surface brightness profile appears to decrease steadily from the core outwards. There is a slight elongation observed, with a deviation from a perfect circular shape.

Evidence suggests the presence of a minor disturbance in its morphology, potentially indicating a past or ongoing interaction or accretion event. There is no discernible tidal tail or other major disruptions to the overall structure. The color appears relatively uniform, with no strong evidence of recent star formation activity. The galaxy appears to be fairly compact in size. 
