The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge that exhibits a yellowish hue, suggesting a population of older stars. The galaxy appears elongated, with its major axis significantly longer than its minor axis, giving it a cigar-shaped appearance. There is a subtle hint of possible disturbance or irregularity in the outer regions of the galaxy, but no clear signs of a major ongoing merger event are apparent. The overall color indicates that star formation activity is likely suppressed, but there might be some low-level star formation occurring based on its bluer color. Its estimated physical size suggests that it is a large galaxy.
