The galaxy presents a morphology that leans towards a smooth profile but exhibits subtle features, potentially indicating the presence of a disk-like structure. It appears to be elliptical, although not perfectly circular. A slight elongation is noticeable, suggesting a possible cigar-shaped structure. The galaxy's overall color suggests a moderate presence of older stellar populations. There is no strong visual evidence of major merger activity, though minor disturbances might be present, indicated by the galaxy's asymmetric light distribution. Star formation rate is low.
