The galaxy exhibits a complex morphology, possibly indicative of an ongoing or recent interaction or merger event. The central region of the galaxy is dominated by a bright, yellowish core suggesting an older stellar population. Extending outwards from this core, a fainter bluish feature is visible, potentially a tidal tail or a disrupted spiral arm. The overall structure appears somewhat irregular, lacking the well-defined spiral arms often seen in undisturbed disk galaxies. There is also a fainter region of disturbed morphology to the lower right of the galaxy. The galaxy is moderately luminous. Based on the tidal tail feature and disturbed morphology, it seems that merging may be the case here.