The galaxy appears as a concentrated elliptical structure. Its overall form is smooth with no easily discernible spiral arms or bar. The light distribution is centrally concentrated, fading gradually towards the outer regions of the galaxy. The color suggests an older stellar population, exhibiting a yellowish-red hue. There's an absence of significant dust lanes or prominent star-forming regions. The galaxy's shape seems fairly regular, without apparent tidal distortions or signs of ongoing major mergers. There might be some minor asymmetry or subtle disturbances, indicating past interactions or minor mergers. Overall, the galaxy is likely an evolved system with a dominant population of older stars and minimal ongoing star formation.
