The galaxy appears as a concentrated, elliptical structure. It exhibits a smooth, largely featureless morphology, lacking prominent spiral arms or a distinct disk. The central region presents a bright, intense luminosity, suggestive of a dense stellar population and potentially a supermassive black hole actively accreting material. The color profile indicates a redder hue, which may be indicative of an older stellar population. The galaxy appears relatively isolated, with no signs of major tidal disturbances or ongoing mergers, although there may be a couple of smaller, more distant galaxies close by. The object appears relatively rounded.
