This galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. There is a slight indication of a disk-like structure, although it is not prominent. The galaxy appears to be fairly circular. Based on the colors presented, the stellar population is likely composed of older stars. There are no immediately obvious signs of a major ongoing merger. However, there may be some minor disturbances in the galaxy's shape or light distribution, potentially indicating a previous interaction or minor merger event. Overall, it is a moderately massive galaxy with low star formation activity.
