The galaxy presents as a somewhat elliptical structure with a smooth, concentrated central bulge. The dominant color of the bulge appears to be a yellow-orange hue, possibly indicative of an older stellar population. Moving outward from the bulge, the disk appears to be relatively featureless, with a blueish tint to one side, suggesting the presence of younger, hotter stars, and ongoing star formation, particularly on the left side of the disk. There are some distortions to the galaxy, with some of the light appearing to extend away from the main body. The galaxy does not appear to be undergoing a major merger, but the minor disturbances suggest that it may have undergone some form of interaction in the past.
