The galaxy presents as a generally smooth, centrally concentrated object with a moderate degree of roundness. There is a central, bright core that appears relatively unresolved in this image. The light profile fades gradually from the core outward, exhibiting no distinct spiral arms or bar structure. There may be a faint, diffuse halo surrounding the brighter central region, but its extent is difficult to ascertain due to the image's limitations. There are no obvious signs of significant tidal disturbances or ongoing major mergers. The overall color appears to be slightly redder, suggesting a population of older stars and a relatively low rate of current star formation. While a disk-like structure may be present, it is not the dominant morphological feature.
