This galaxy presents as a relatively smooth, elliptical morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in intensity towards the outer regions. There are hints of a slight elongation, suggesting it may be more lenticular than perfectly spherical. The dominant color is a yellowish-white, indicative of an older stellar population, possibly dominated by evolved red giant stars. The lack of distinct blue regions suggests a low rate of ongoing star formation. No prominent spiral arms or dust lanes are visible within the resolution of the image. No major signs of gravitational disturbance are apparent in the immediate vicinity of the galaxy.
