This galaxy appears to be a relatively smooth, elliptical system. The light profile is centrally concentrated, exhibiting a bright core that gradually fades towards the outer edges. There is no evidence of prominent spiral arms or a distinct disk structure. The overall shape is generally round, with a slight deviation towards an elongated form. There are no signs of major mergers or significant tidal disturbances, although subtle asymmetries could indicate minor interactions in its past. The color index suggests a population of older stars, with a relatively low rate of ongoing star formation. The estimated size indicates that it is a moderately sized galaxy.
