The galaxy presents a complex morphology, suggestive of ongoing or recent interaction. The central region displays a bright, moderately sized bulge. The surrounding disk shows evidence of distortion, with some asymmetry in its overall shape. Faint, diffuse spiral arms appear to originate from the core region, although their structure is irregular and not well-defined. A significant portion of the galaxy's light is concentrated in a central region, but there are disturbances in the disk of the galaxy that indicate a possible merging event or tidal interactions with another galaxy. There is no strong bar structure visible. The galaxy exhibits a generally blue color, indicative of ongoing star formation.
