The galaxy exhibits a central, bright core suggesting a high concentration of stars or an active galactic nucleus. The light profile appears relatively smooth, indicating a lack of prominent spiral arms or distinct features typically seen in spiral galaxies. The general shape is somewhat elongated with a fairly compact, elliptical morphology. A diffuse halo surrounds the central region, fading gradually into the background sky. There appears to be some dust obscuration, though it is not readily apparent in this particular image. The color gradients within the galaxy show a bluer hue near the center and a more red color in the outer regions. There are some small regions that show evidence of minor tidal interactions, such as streams of stars. There is a likely interaction that has happened, but the galaxy has returned back to its original shape due to a lack of any clear features.
