This galaxy exhibits a morphology suggestive of an ongoing merger event. The system appears to consist of two distinct components, each with a relatively smooth appearance. The primary component displays a yellowish hue, potentially indicating an older stellar population. The secondary component appears bluer, suggesting the presence of younger stars and possible star formation activity. There is a faint connection of light between the two components that further indicates that this galaxy is undergoing a merger. The overall structure is somewhat irregular, deviating from a well-defined spiral or elliptical form. The light profile fades gradually towards the outer edges, lacking a sharp boundary.
