The observed galaxy exhibits a somewhat amorphous structure with subtle features suggestive of gravitational interaction or recent merger activity. The central region shows a slightly smoother morphology. The light distribution indicates a concentration of older stars in the core, giving a yellowish hue. Extending outwards from the center, bluer tinges are apparent, hinting at the presence of younger stellar populations. These bluer regions could also be indicative of ongoing star formation. Faint disturbances are seen in the outer regions of the galaxy, though these could also be effects of light scattering or an artifact. Overall, the galaxy's morphology suggests a system undergoing some form of dynamic evolution, where there may have been recent interactions.
