The galaxy exhibits a generally smooth morphology, suggesting it is an early-type galaxy, possibly an elliptical or lenticular. The light profile appears concentrated towards the center with a gradual fade in intensity moving outwards. The galaxy exhibits a slight elongation, appearing more in-between of round and cigar-shaped. A distinct feature is the presence of a minor disturbance, which may indicate a possible interaction. Given the overall light distribution and morphology, this galaxy is likely relatively massive, exhibiting moderate ongoing star formation.
