This galaxy presents a complex morphology, possibly indicative of an ongoing or recent interaction. It exhibits a bright, relatively smooth core, which appears somewhat elongated. A distinct, less luminous component is visible, offset from the primary core. This secondary feature displays bluer coloration than the primary body, suggesting a younger stellar population or differing dust content. Faint tidal features may extend from the main galaxy, further supporting the possibility of a gravitational interaction. The overall shape is irregular, lacking a clear spiral or elliptical structure. Based on its color, this galaxy seems to be composed of both an older population of stars (yellowish) and a younger one (bluish), implying an active star formation phase may recently have occurred or still be ongoing. There is no single, clear nucleus. 