The galaxy presents as a largely smooth, elliptical form. Its shape is intermediate between round and cigar-shaped. A central bulge dominates the structure, exhibiting a yellow-orange hue, suggesting an older stellar population. There is some indication of a faint disk, possibly composed of younger stars, exhibiting a very faint bluish tint toward the outer edges of the galaxy. No significant signs of major mergers are detected. There is a hint of minor disturbance within the galaxy. The galaxy’s apparent size is small, suggesting either a physically compact object or substantial distance. The galaxy appears to be relatively isolated, with no obvious nearby interacting companions in the immediate vicinity.
