The galaxy presents an overall smooth morphology, lacking discernible spiral arms or a prominent disk structure. The central region exhibits a concentrated brightness, suggesting a significant bulge component. There appears to be a color gradient, with the core showing a more yellow-orange hue, potentially indicating an older stellar population. A fainter, slightly bluer region extends from the main body, hinting at possible tidal interactions or recent merger activity, although the overall structure doesn't exhibit strong distortions typically associated with major mergers. The roundness of the galaxy is relatively high. Star formation rate may be low.