The galaxy appears as a centrally concentrated, smooth object, likely elliptical in nature. It exhibits a notable color gradient, transitioning from a bright, yellowish-orange core to a dimmer, bluer outer halo. The isophotes appear generally round, although some slight deviations from perfect circularity are present. There is no readily apparent spiral structure or dust lanes visible. There are very faint, small disturbances near the halo, hinting that the galaxy may have had a minor merger event sometime in the past. Overall, the galaxy exhibits an evolved stellar population, consistent with low current star formation and the red color of the core, suggesting a prevalence of older, redder stars in this central region.
