The galaxy presents as a relatively compact object, exhibiting a centrally concentrated light profile. The core region shows a bright, almost unresolved, emission. The overall color appears bluish-white, suggesting the presence of a significant population of young, hot stars or a strong central ionizing source. Some minor disturbances or tidal features may be present. There is potential evidence of some minor morphological disruption, but the overall structure remains largely intact. There could also be an active galactic nucleus, as indicated by the color.
