The galaxy exhibits a pronounced elongated, cigar-like morphology, indicating a possible elliptical or lenticular classification. There is a bulge in the center with an elliptical shape. Overall, the galaxy appears to be relatively smooth in texture, however there are some irregularities and disturbances on the left side. There also appears to be another object on the left side that could be a star or dwarf galaxy that may be the cause of the galaxy's disturbed nature. There is a color gradient with the central region appearing yellow/orange, and the outer regions appearing more bluish. Given these characteristics, the galaxy could be undergoing some form of interaction or disturbance, potentially a minor merger event. Overall, the galaxy has a high estimated mass and moderate star formation rate.
