The galaxy appears as a singular, centrally concentrated object. Its morphology is predominantly smooth, exhibiting a generally elliptical shape. The light distribution suggests a well-mixed stellar population, lacking any discernible spiral arm structure or significant dust lanes. There is a subtle elongation in the galaxy's form, deviating slightly from a perfect circular shape. The galaxy displays a moderately red color, suggestive of an older stellar population and reduced ongoing star formation activity. Close inspection reveals a slight irregularity in its outer regions, possibly indicative of minor gravitational interactions or past mergers. However, the core region appears undisturbed.
