The galaxy presents as a flattened, elliptical morphology. Its light profile appears smooth, lacking any distinct spiral arms or bars. The core region exhibits a concentrated luminosity, suggesting a high stellar density, possibly indicating the presence of a supermassive black hole. Moving outward from the core, the light gradually fades. There is faint evidence of a disk, though the image is not precise enough to confirm this. There is no visible sign of any ongoing major mergers or significant tidal disturbances in the image, and no clear evidence of active star formation regions. The galaxy's red hue points to a population of older stars, potentially indicating a lower current star formation rate. Overall, this galaxy seems to be relatively evolved, with a large stellar mass.
