The galaxy presents as a centrally concentrated system with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Surrounding the core is a more diffuse region that appears to be transitioning into a reddish-orange color. The overall shape appears to be somewhere between round and slightly elliptical. There are no obvious signs of strong spiral arm structure or a well-defined disk. The outer regions show faint color variations. No signs of major mergers or tidal disturbances are readily apparent, though minor irregularities cannot be ruled out at this resolution. The galaxy seems relatively isolated in its immediate environment, but the low quality of the image may make it hard to spot minor disturbances.
