The galaxy presents a somewhat smooth, elliptical appearance, although there is evidence of a possible disk structure. A bright central bulge dominates the overall luminosity profile. The galaxy is relatively round in shape. There is a hint of blue color, particularly in areas outside of the central bulge, suggesting the presence of a younger stellar population and ongoing star formation, albeit potentially at a moderate rate. Based on observed irregularities, it is likely that the galaxy has undergone a minor disturbance event sometime in the past.