The galaxy presents as a dominant, roughly circular, yellowish light distribution, suggestive of an elliptical galaxy or the bulge component of a spiral. There is a secondary, smaller, reddish component, possibly indicating a region of active star formation or a smaller, interacting galaxy. The overall light profile appears smooth, lacking the distinct spiral arm structures or irregular features often associated with late-type galaxies. There's a slight asymmetry suggesting a potential minor interaction or internal disturbance. The redder color of the secondary component suggests an older stellar population, heavily dust-obscured region, or a higher redshift object.
