The galaxy exhibits a somewhat lenticular morphology, displaying a central bulge with a comparatively faint disk structure. There appears to be a lack of well-defined spiral arms. The nucleus is bright, concentrated, and appears slightly offset from the geometric center of the disk. Color gradients across the galaxy show a bluer central region transitioning to redder outer edges. This may indicate ongoing star formation in the core, with older stellar populations dominating the outskirts. There is a slight suggestion of a tidal tail or streamer emanating from one side of the galaxy, hinting at a possible past or ongoing interaction with another galaxy. The overall structure suggests a galaxy undergoing some form of disturbance or transformation. 
