This galaxy exhibits a complex morphology, potentially indicating an ongoing or recent interaction. The overall structure appears somewhat disturbed, deviating from a regular elliptical or spiral form. There is evidence of multiple luminous knots or clumps, suggesting regions of active star formation. These regions display a range of colors, with some appearing more yellowish and others showing a bluer tint, potentially indicating different stellar populations or dust extinction levels. A faint, diffuse halo surrounds the central regions, and a possible tidal tail extending from the main body. The general appearance indicates a moderately massive galaxy experiencing a high degree of starburst activity. There is clear evidence of an ongoing interaction and the disturbance of the main body.
