The galaxy exhibits a generally smooth morphology, with a dominant spheroidal component. The light distribution appears concentrated towards the center, exhibiting a bright core. The isophotes are moderately elliptical, but not highly elongated. The galaxy displays a yellow to orange color, suggesting a stellar population dominated by older stars. There is no indication of prominent spiral arms or significant dust lanes. The overall structure suggests an early-type galaxy, likely an elliptical or lenticular system. There is very weak possible evidence of a minor disturbance in the outer regions of the galaxy, but no evidence for an ongoing merger, although this is difficult to determine from the resolution of the image.