The galaxy presents as a diffuse, elliptical structure. Its light distribution appears relatively smooth, with a centrally concentrated luminosity that decreases gradually towards the outer regions. A subtle color gradient is discernible, exhibiting a bluer hue towards the central region of the galaxy, suggestive of a population of younger, hotter stars. The outer edges appear redder, possibly indicating a greater proportion of older, cooler stars. The galaxy's overall shape is elongated, with a slight flattening, deviating from a perfectly circular morphology. There's no clear evidence of spiral arm structures or distinct dust lanes. The galaxy appears to be a relatively isolated system, showing no signs of major interactions or ongoing mergers with other galaxies based on its current morphology in this image.
