The galaxy presents as a single, somewhat disturbed object with an elongated morphology. It appears to be composed of two distinct concentrations of light, suggesting a possible merging event or a galaxy with a prominent tidal tail. The primary, brighter concentration exhibits a more reddish-orange hue, potentially indicative of an older stellar population or significant dust obscuration. The secondary concentration of light, located to the upper left, presents a slightly more yellowish color, hinting at a potentially younger stellar population or less dust. The galaxy is neither perfectly elliptical nor a clear spiral, and appears to be in a state of interaction with the surrounding environment.
