The galaxy presents as a smooth, centrally concentrated object. It exhibits a notable elongation, appearing cigar-shaped. The color profile suggests a dominant population of older stars, indicated by the yellowish hue. There is a hint of bluer color towards the edges, suggesting some ongoing, but likely limited, star formation activity. No distinct spiral arms or bar structures are discernible; the overall morphology is suggestive of an elliptical or lenticular galaxy. No obvious signs of a major merger event are visible, though there may be a very slight asymmetry or minor disturbance on one side.
