The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a high concentration of light toward the center. It exhibits a generally rounded morphology, lacking the distinct spiral arm structures characteristic of late-type galaxies. The light distribution suggests a relatively old stellar population, with the redder hues predominating. There is a subtle hint of disturbance, possibly from a minor interaction or past merger event, but the overall structure remains largely undisturbed. The galaxy is a luminous object, with an estimated size that indicates it may be a relatively large galaxy within its population. Considering its color, it likely has a low rate of ongoing star formation.
