The galaxy presents as a relatively smooth and elliptical structure. The main body exhibits a pinkish-red hue, suggesting the presence of an older stellar population and perhaps some dust obscuration. The galaxy's shape appears elongated, with the major axis significantly larger than the minor axis. There's a central concentration of light, possibly indicating a bulge or a core region. There is also a ring-like structure. Evidence for active star formation is not immediately apparent from the visual data. There may be some disturbances present within the galaxy, although they are minor. There are no immediately obvious signs of ongoing mergers or interactions.
