The galaxy appears to be a relatively bright, disk-shaped system. It exhibits a smooth, elliptical morphology, suggesting a dominant spheroidal component. The central region displays a reddish-yellow hue, potentially indicative of an older stellar population. Surrounding the core is a greenish-yellow disk, possibly indicative of ongoing star formation within spiral arms or rings that are not clearly resolved in this image. There is no evidence of major tidal disturbances or ongoing mergers, although subtle asymmetries might be present, requiring higher resolution imaging for confirmation. Overall, the galaxy presents as an evolved system with a moderate level of star formation.
