The object appears to be a galaxy displaying signs of an ongoing or recent interaction. It is characterized by a mostly smooth, rounded morphology, with a noticeable deviation from perfect symmetry indicating possible disturbances. The primary structure exhibits a bright, concentrated core region. The overall color profile suggests a relatively higher population of older stars, but there are regions showing bluer emissions indicative of younger star formation, particularly around the central regions. There is also a second region which appears to be connected to the primary region. Both have irregular shapes and distributions of light, suggestive of tidal interactions. Overall, the galaxy appears to be in a transitional phase in its evolution.
