The galaxy presents a generally smooth, elliptical morphology. The color profile indicates a substantial population of older stars, giving it a reddish-gold hue. There is a slight elongation, but overall, the galaxy appears quite round. The light is concentrated towards the center, suggesting a dense core. No distinct spiral arms or prominent dust lanes are discernible. There are also slight indications of minor disturbances in the evenness of the light emitted, which could be evidence of interaction with another galaxy, although this could also be due to artifacts in the imaging. Overall, the galaxy's color and morphology suggest that the galaxy is a relatively massive, quiescent system with a suppressed star formation rate.
