The galaxy presents as a somewhat elongated, disk-like structure with a moderately bright central bulge. The color gradient suggests a redder core transitioning to bluer outer regions, potentially indicative of ongoing star formation in the periphery.  There is a subtle, yet noticeable asymmetry in the galaxy's structure, possibly the result of a past or ongoing minor interaction, although no obvious tidal features or strong disturbances are immediately apparent. The overall morphology suggests a spiral galaxy, seen at a moderate inclination, yet it also exhibits features consistent with S0, a disk galaxy with little to no spiral arms.
