The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated brightness, suggesting a high stellar density and potentially a supermassive black hole at the galactic nucleus. There is an apparent absence of prominent spiral arms or a well-defined disk structure. The light distribution appears relatively uniform and rounded. While the image quality does not allow for definitive assessment, there may be minor disturbances present in the outer regions, potentially indicative of past minor mergers or tidal interactions. Overall, the galaxy appears as a relatively isolated system, without significant evidence of ongoing major mergers or interactions. The color profile suggests the presence of a stellar population that is actively forming stars.
