The galaxy appears to be an elongated elliptical type. Its light profile is smooth and concentrated, with a gradual fading towards the edges, indicating a lack of distinct spiral arms or prominent features. The galaxy exhibits a reddish-yellow hue, suggesting an older stellar population with a low rate of ongoing star formation. The galaxy presents a cigar shape, appearing significantly longer than it is wide. There is no evidence of major mergers or significant tidal disturbances; the overall morphology appears relatively undisturbed. 
