The galaxy appears as a centrally concentrated, smooth object with a relatively symmetrical and rounded morphology. Its color is predominantly yellowish, suggesting a population of older stars. There is a lack of any apparent spiral arm structure or distinct features such as dust lanes or star-forming regions. The galaxy exhibits a gradual decline in surface brightness from the core outwards, indicating a smooth distribution of stellar mass. There are no signs of tidal disturbances or ongoing mergers, but it's possible there is minor disturbance. Overall, the galaxy appears to be an elliptical or lenticular type, likely a massive and relatively quiescent system with minimal ongoing star formation.
