The galaxy presents as a relatively smooth, centrally concentrated structure with a moderate degree of ellipticity. The core appears yellowish-orange, potentially indicating a population of older stars. Fainter, diffuse, blue-green emission extends outwards from the core, suggesting the presence of some younger stellar populations and ongoing star formation, although at a modest rate. No distinct spiral arms or bar structures are readily apparent. There are no obvious signs of a recent major merger, although some minor asymmetry or disturbance in the outer regions cannot be ruled out. The overall morphology is consistent with an intermediate-type galaxy, possibly an early spiral or a lenticular galaxy with some residual star formation.
