The galaxy presents as a single, somewhat amorphous light source. There appears to be a high degree of radial concentration towards a relatively bright core, exhibiting a yellow-white hue, suggesting a population of older stars. Extending outward, there are some hints of blue-ish light, which could indicate star forming regions, although this is less distinct. The overall shape appears slightly elongated. The galaxy shows no distinct spiral arm structures and appears to be in a non-quiescent state, likely undergoing some sort of interaction or morphological disturbance.
