The galaxy presents as a slightly elongated, elliptical-like structure. The central region appears bright and concentrated, exhibiting a smooth texture. Moving outward from the core, the luminosity gradually diminishes into the surrounding space. There appears to be a slight asymmetry in the outer regions. While the overall form is suggestive of a smooth system, some subtle distortions indicate possible interactions. These irregularities could represent the remnants of a minor merger event. The color profile is relatively uniform, suggesting a population of older stars, with the exception of some minor disturbances possibly containing some young stars.
