The galaxy presents as a somewhat elliptical morphology, exhibiting a central, brighter bulge region. The overall color appears to be slightly redder in the bulge, suggestive of an older stellar population. Moving outward from the core, the galaxy transitions to a fainter, bluer disk. While the disk is not clearly resolved into spiral arms, there is a hint of a slightly irregular structure. The edge-on presentation may contribute to the observed features and overall faintness of the system. There appear to be some minor disturbances present, indicating a possibility of a small interaction. The overall smoothness of the system suggests that any merger event is unlikely to be recent or significant.
