The galaxy presents as a diffuse, centrally concentrated object. There is some evidence of a disk structure. The galaxy exhibits a noticeable color gradient, with a yellower/gold hue concentrated in the central regions, transitioning to a bluer outer halo. This suggests older stellar populations towards the center and younger, bluer stars in the surrounding regions. The morphology appears disturbed with irregularities in its shape, possibly indicative of an ongoing or recent interaction or merger event. There is some evidence of tidal tails or other extended structures. A small, faint, diffuse arm extends slightly to the right from the center, suggestive of a disruption. The object does not present a perfectly smooth appearance, and may indicate the presence of irregular features and faint structures. Overall, it appears to be a somewhat perturbed disk galaxy, possibly undergoing a merger or interaction, exhibiting a mix of stellar populations.
