The galaxy exhibits a complex morphology, showing signs of a possible interaction or merger. The core region presents a yellowish-orange hue, potentially indicative of an older stellar population and/or significant dust obscuration. Extending from this central region is a fainter, bluish component, which may represent areas of more recent star formation. This bluish region appears somewhat irregular and disrupted, lending support to the idea of ongoing gravitational disturbance. The overall shape is elongated, with deviations from a perfectly elliptical structure, hinting at tidal features or ongoing accretion. There is no clear spiral arm structure visible. The galaxy appears relatively massive, with a suppressed star formation rate.
