The galaxy presents a moderately elliptical morphology, appearing cigar-shaped. There is a central bulge region that exhibits a yellowish hue, likely indicating an older stellar population. This area transitions to a bluish area on one side of the galaxy. This suggests ongoing star formation in that region, or possibly the aftermath of a merger event causing a disturbance in the galaxy's structure. Overall, the galaxy shows signs of a relatively quiescent star formation rate given its mass, but the bluer area indicates that some amount of recent star formation has occurred. It does not seem to be undergoing a major merger. There may be some sort of minor disturbance.
