The galaxy appears to be in the midst of a significant interaction, potentially a merger. There are two distinct, yet connected components visible. The upper component shows a bluish hue, indicative of possible ongoing or recent star formation. The lower component is more concentrated and exhibits a yellower tint, possibly suggesting an older stellar population. The overall shape is disturbed and irregular, deviating from a regular spiral or elliptical form. There is a faint tidal tail extending outwards. The system is reasonably luminous, suggesting a substantial stellar mass. There appears to be a moderate level of star formation occurring within the system.