The galaxy appears as a relatively compact object with a concentrated, bright central region. Surrounding this central concentration, a faint, diffuse halo is visible, extending outwards. The color profile suggests a possible redder outer region when compared to the bluer center. The observed structure indicates potential disturbances or interactions, possibly in the form of tidal features, though these are subtle. There is not any significant evidence for spiral arm structures, though there are some irregular features in the outer regions. The appearance indicates a galaxy undergoing, or having recently undergone, some form of significant gravitational interaction.
