This galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated light distribution. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy is relatively rounded in shape, deviating only slightly from a perfect circle. There is a slight color gradient, transitioning from a more yellow-reddish hue at the core to a slightly bluer tint in the outer regions. There is no indication of a major ongoing merger event, nor significant tidal features or strong disturbances. It looks like a galaxy that has exhausted most of its gas reservoir for star formation.
