The galaxy exhibits a generally spheroidal morphology, with evidence of a central bulge that dominates the visual appearance. The light from this bulge appears consistent with an older stellar population. There is also an asymmetry visible, perhaps due to a past or ongoing interaction. Some faint, diffuse structures surround the central region, suggesting tidal debris or disrupted spiral arms. The overall color profile indicates a moderately evolved system, with a moderate amount of star formation. Signs of disturbance indicate a possible merger event. 
