The galaxy exhibits a centrally concentrated luminosity profile, appearing relatively smooth. The shape is somewhat elliptical, with a noticeable difference between its major and minor axes. Color gradients are subtle, with a suggestion of bluer hues in the outer regions and a yellower, possibly older stellar population concentrated towards the center. There seems to be a weak disk. There are no distinct spiral arms or prominent dust lanes, indicating a more evolved system that may be approaching the red sequence. The general morphology is consistent with an early-type spiral or a lenticular galaxy. There are also no indications of recent or ongoing major mergers. There may be some minor disturbances. Overall, the galaxy presents as a quiescent system with a significant fraction of its stellar mass likely in an older population.
