The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth light distribution with no apparent spiral arms or bar structure. It is centrally concentrated, with a bright core that fades gradually towards the outer regions. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or major mergers. There are hints of some surrounding dust or gas, which could possibly hint at a past interaction or ongoing internal processes. The galaxy displays a yellowish-white color, suggesting an older stellar population. Overall, it appears as a relatively quiescent galaxy dominated by evolved stars and with a low rate of current star formation.
