The galaxy appears to be elliptical or lenticular in morphology, exhibiting a relatively smooth and concentrated light profile. There is no obvious presence of spiral arms or a prominent disk structure. The galaxy is dominated by yellowish-white light, which may indicate a population of older stars with lower rates of current star formation. The color suggests that this is a galaxy with a significant fraction of evolved stellar population. There are some subtle color variations, with slightly greener hues on the outskirts, which could suggest some residual or recent star formation activity or contribution from ionized gas, though the dominant appearance is generally smooth and consistent with an older population. There is no obvious indication of a major merger event or significant tidal disturbances.
