The galaxy presents an elongated, cigar-shaped morphology, suggesting it is likely an elliptical galaxy viewed at an angle. It exhibits a smooth, relatively featureless appearance, indicating a lack of significant spiral arm structure or dust lanes. The color gradient transitions from a yellowish core to a slightly bluer periphery. This color profile could suggest a centrally concentrated older stellar population with younger, bluer stars distributed further out. No signs of any major mergers can be detected, but it could be undergoing a minor disturbance.