The galaxy exhibits a concentrated, elliptical morphology, appearing relatively smooth with minimal discernible substructure. The light distribution is dominated by a bright, centrally located bulge region, exhibiting a color gradient that shifts from a yellow-white core to a more reddish hue in the outer regions. This suggests an older stellar population throughout the main structure of the galaxy. There is a slight extension or tidal feature to one side of the galaxy, it is unclear whether this is due to an ongoing interaction or a remnant of a past merger event. Overall, the galaxy presents as a quiescent system with signs of potentially past interactions.
