The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated brightness profile that diminishes gradually outward. It appears to be elliptical in shape but not extremely so. There are no readily apparent spiral arm structures or significant dust lanes visible in the image. The galaxy appears to have a dominant, rounded bulge component with a diffuse halo. The color distribution suggests a population of older stars, especially within the core, as indicated by its reddish hue, which fades toward the edges of the galaxy. There is only minor evidence of disturbances or interactions with neighboring galaxies, and the overall structure appears relatively undisturbed.
