This galaxy presents as a centrally concentrated, elliptical-like system. The primary body exhibits a smooth, diffuse light profile with a noticeable lack of distinct spiral arm structures or prominent dust lanes. The central region displays a slightly brighter, yellowish hue, possibly indicating a concentration of older stellar populations and/or dust obscuration. This central concentration is quite compact, likely representing a bulge component.

The overall shape appears largely spheroidal. There's a very subtle extension along one axis. The galaxy doesn't appear to be undergoing a major merger event, though there is some slight asymmetry to the distribution of light, hinting at a possible minor interaction or internal disturbance. The overall color gradient suggests a potentially evolved system with relatively low levels of ongoing star formation.
