The galaxy presents as a centrally concentrated, diffuse object. It displays a moderate degree of ellipticity, appearing somewhat elongated, though it leans toward being round. The core region exhibits a yellowish hue, indicating a likely concentration of older stellar populations. Extending outward from the core, a faint, blueish halo is observed, potentially suggesting the presence of younger stars or ongoing star formation, though it is not very active. There is some evidence of minor morphological disturbance, with possibly a slight tidal feature but this could also be dust. The galaxy's overall structure appears relatively smooth, suggesting a later stage of its evolution. It does not clearly display prominent spiral arms or a distinct disk.
