The observed galaxy presents a generally smooth morphology, albeit with subtle features suggesting potential disturbances. The central region exhibits a higher concentration of light, indicative of a galactic nucleus or bulge. Extending outwards from the core, a faint disk-like structure is barely visible, suggesting a spiral or lenticular morphology. However, the overall light distribution is somewhat irregular, hinting at possible past interactions or mergers. The color profile appears relatively uniform, implying a homogenous stellar population with a mix of young and old stars. The apparent size of the galaxy is small, and the low surface brightness suggests that it is either a dwarf galaxy or a more massive galaxy at a significant distance. There are suggestions of disturbed morphology as well, possibly indicating an ongoing merger.
