The galaxy appears to be relatively small and compact. It exhibits a roughly circular morphology, although there are some subtle irregularities in its shape. The galaxy's core region shows a bright, concentrated luminosity, suggesting a possible active galactic nucleus or a dense stellar population. Surrounding the core, there's a faint, diffuse halo of light extending outwards. The color distribution seems heterogeneous, with a central bluish-white hue transitioning to greenish and reddish tones in the outer regions, indicating varying stellar populations and potentially ongoing star formation. There is a slight indication of a possible tidal tail, suggesting that it may have experienced gravitational interactions with another galaxy in the past. This evidence may also suggest that it is potentially merging. The galaxy does not appear to have well-defined spiral arms or a distinct disk structure.
