The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that gradually fades into a diffuse outer halo. The color profile suggests an older stellar population, with a yellowish-white hue dominating the central regions, indicative of evolved stars. There's a slight elongation along its major axis, giving it a cigar-like appearance, with a hint of bluer colors towards the edges, which might indicate pockets of recent, but limited, star formation. No distinct spiral arms or prominent dust lanes are discernible at this resolution, reinforcing the impression of a galaxy that has largely exhausted its gas reservoir. It appears relatively isolated.
