The galaxy presents as a diffuse, low-surface-brightness object. There appears to be a faint, somewhat elongated central bulge with a nebulous, extended halo or disk surrounding it. The overall structure lacks distinct spiral arms or a well-defined shape, exhibiting a rather amorphous appearance. The light distribution is not uniform, but appears mottled or patchy throughout the galaxy, indicating possible areas of differing stellar populations or dust obscuration. A hint of possible tidal interaction or minor disturbance appears evident in a slightly asymmetric structure of its outer halo. The overall color is mostly muted, suggesting a population of older stars, with a potential for the presence of some younger, hotter stars in certain regions based on their slightly brighter and bluer light. There might be ongoing or recent star formation activity within the galaxy, concentrated in some specific regions.
