This galaxy exhibits a moderately concentrated central region with a soft, diffuse halo extending outwards. There is a slight hint of asymmetry in the halo's distribution, with a somewhat elongated structure. The color profile indicates a complex mix of stellar populations. The core appears to be primarily composed of older stars. Evident from the redness, there are areas of intense star formation. These regions are likely associated with ongoing or recent interactions, potentially a minor merger event contributing to the overall morphology. Overall, the galaxy presents a disturbed appearance, suggesting a history of interactions or internal processes that have shaped its current form.
