The galaxy exhibits a complex morphology, suggesting a possible ongoing or recent merger event. The core region displays a bright, concentrated luminosity, possibly indicative of an active galactic nucleus or a region of intense star formation.

A faint, extended structure is visible on one side of the central core, with the potential to be tidal debris. It appears distorted, deviating from a smooth, elliptical shape. It is also possible that this could be an interacting smaller galaxy.

Based on the color gradients, the stellar population appears to vary across the galaxy. The core is characterized by bluer light, while more distant regions are redder, implying different ages or metallicities.
