The galaxy appears as a relatively small, but noticeably extended object. Its central region is bright and concentrated, exhibiting a near-spherical morphology with a slight elongation evident along what appears to be a major axis. The overall color appears to be a slightly blueish-white hue, indicative of a stellar population with a range of ages, including some younger, hotter stars. The galaxy lacks a strong spiral arm structure, but it may have some subtle features that suggest a disk component viewed at a high inclination angle. There is a possible indication of a faint, asymmetrical structure extending from the central region.
