The galaxy presents as an elliptical or lenticular morphology. It exhibits a smooth, centrally concentrated luminosity profile with a high degree of central concentration and little discernible internal structure such as spiral arms or dust lanes. The galaxy displays a yellowish-orange color, suggesting a population of older stars and a low rate of ongoing star formation. The overall shape is approximately round. There is no apparent evidence of recent or ongoing major merger activity, although faint asymmetric features might suggest minor tidal disturbances or interactions. The galaxy appears relatively isolated in its immediate environment.
