The galaxy appears to be undergoing a merger. There is a primary, somewhat smoothed spheroidal component with a yellowish hue, suggestive of an older stellar population. A secondary, smaller component is visible with a bluer color, hinting at ongoing star formation. Evident disruption in the overall morphology is observable, with what appears to be a tidal tail extending from the primary component, pointing towards the secondary component. The galaxy is not perfectly rounded but rather appears somewhat elongated and disturbed, indicative of gravitational interactions and potential tidal forces at play between the merging galaxies. Overall, the system is not fully relaxed and possesses features characteristic of an ongoing merger event.
