The galaxy presents as a largely smooth, centrally concentrated structure. There is a distinct lack of well-defined spiral arms or a prominent bar. The central region displays a bright, diffuse glow, potentially indicating a substantial bulge component. The galaxy exhibits a generally elliptical morphology, with the majority of its light distributed in a roughly circular pattern. The overall color appears to be intermediate, with a slight reddening towards the core, suggesting a population of older stars residing primarily in the center. There are hints of slightly bluer, potentially younger stellar populations in the outer regions of the galaxy, although these features are subtle and lack the defined structure associated with active star formation regions. There might be some minor interaction or disturbance in the galaxy's structure, but overall it does not appear to be in a state of major merging or tidal disruption.
