The galaxy presents a generally smooth morphology, with an apparent lack of distinct spiral arms or a pronounced bar structure. It exhibits a concentrated central bulge that appears slightly elongated in shape. Two dominant color gradients are observed within the galaxy. The central region displays a reddish-orange hue, possibly indicating an older stellar population or significant dust obscuration. A more bluish component is visible adjacent to the center, suggestive of younger stars or a region of ongoing star formation. The galaxy's overall shape is predominantly round. The galaxy appears to show signs of possible tidal disruption or an interaction with a companion, although this is not definitive. There may be some minor disturbance to its shape, but it is most likely not involved in a major merging event.
