The galaxy presents a morphology that appears to be intermediate between a purely elliptical and a disk galaxy. The central region exhibits a relatively smooth, concentrated luminosity profile, indicative of a spheroidal component. The overall shape is neither perfectly circular nor significantly elongated, displaying a degree of intermediate ellipticity. Faint, diffuse features suggest the presence of a possible disk or tidal disturbance. There appears to be some evidence of a possible minor merger event or tidal interaction.
