The galaxy appears to be a single, somewhat elliptical, though largely rounded object. The main body presents a smooth, concentrated light profile with a noticeable radial gradient indicating brightness decreasing from the core outward. Coloration is primarily reddish, suggesting an older stellar population and/or significant dust obscuration. There is no strong evidence of spiral arms or a distinct disk structure visible in this imagery. Some irregularity can be observed, and there is a possible indication of a minor disturbance within the galaxy's structure, suggesting potential tidal interactions or recent minor merger event. There are no apparent tidal tails or bridges, nor any clear evidence of a major merger event. It could be a relatively undisturbed elliptical galaxy.
