The galaxy presents as a somewhat smooth, disk-like structure with a bright, concentrated central bulge. The overall color appears yellowish-white, suggesting a population of older stars dominating the light output. There is a subtle flattening of the disk, with possible faint spiral arm structures hinted at within the extended, diffuse outer regions. Minimal dust lanes are discernible within the disk, suggesting the galaxy is undergoing relatively little current star formation. There are slight disturbances to its shape and faint visual signs of a tidal interaction, such as minor asymmetries in the outskirts, possibly indicative of a past or ongoing minor merger event.
