The observed galaxy appears to be relatively compact, exhibiting a somewhat amorphous morphology. The central region displays a high surface brightness, indicative of a concentrated core. Fainter extensions are visible, hinting at a possible disk or tidal features. These extensions appear asymmetrical, suggesting potential gravitational interactions or disturbances. The color profile indicates a gradient, with the central region appearing bluer, possibly due to a younger stellar population, and the outer regions exhibiting a redder hue. Overall, the galaxy appears to be a moderately complex system with subtle structural features. Further investigation is warranted to determine the nature of the faint extensions and the possible presence of a disk.
