The galaxy presents a complex morphology. The central region exhibits a smooth, concentrated bulge, appearing yellowish, indicative of an older stellar population. Extending outward from this central bulge are fainter, bluish extensions, possibly indicative of ongoing or recent star formation within a disturbed disk. There seems to be some degree of tidal disruption or ongoing interaction with a companion, as indicated by the irregular shape and extended features on one side. The shape is mostly rounded, but there is some elongation, possibly in cigar shape. There is a strong possibility of a major merger or interaction causing this.
