The galaxy presents as a relatively smooth and rounded structure. The core region exhibits a concentrated, bright emission, suggestive of a significant population of older stars. The light fades gradually towards the outer regions. No obvious spiral arm structures or distinct features are visible; instead, the overall morphology appears largely spheroidal. There are no readily apparent signs of any recent major mergers or significant tidal disturbances; however, there is a chance of a minor disturbance. The color profile suggests a relatively evolved stellar population throughout, with a slightly redder hue dominating the galaxy's overall appearance. The galaxy presents a smooth appearance, with 80% of surveyed citizens agreeing. The galaxy is round and has no cigar shape to it.
