The galaxy presents a generally smooth appearance, with a slightly elongated, cigar-like shape. The light distribution is centrally concentrated, but appears to be somewhat disrupted. It exhibits a notable redder color profile, suggesting an older stellar population and relatively low ongoing star formation activity. No distinct spiral arms or bar structures are clearly discernible. There is a possible indication of a faint tidal feature or minor disturbance, which might imply a past interaction or minor merger event. The overall morphology suggests it could be an elliptical galaxy. 
