The galaxy presents as a moderate-sized extended object with an approximate elliptical morphology. The central region appears more luminous and concentrated, exhibiting a yellowish-white hue, suggesting a population of older stars. Extending outwards from the core, the galaxy appears more diffuse. There's some evidence of tidal disturbances, potentially indicating a past or ongoing merger event. The outer regions show a bluer color, which might signify the presence of younger stellar populations. The galaxy does not seem to have a clearly defined spiral structure. Overall, it exhibits properties consistent with a disturbed galaxy.
