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 structure, without prominent spiral arms or distinct dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer edges. The color profile indicates a redder hue overall, which is consistent with an older stellar population and suppressed star formation. There is some indication of minor disturbances in its shape which may indicate interaction with a smaller nearby galaxy. 
