The galaxy presents as a relatively smooth, elliptical object with a noticeable central bulge. The light profile appears to be concentrated toward the center, suggesting a higher density of stars in the core. The overall color is yellowish-orange, indicative of an older stellar population with fewer hot, young blue stars, and a dominance of cooler, redder stars. There's a slight elongation in the galaxy's shape; it is more "in between" than either perfectly round, or "cigar" shaped. No distinct spiral arms or dust lanes are discernible. The outer regions fade gradually into the background, with no sharp edges. There is no clear evidence of major mergers or tidal disturbances affecting the galaxy's overall structure. Slight bluer hue around the edges indicates possible small amounts of star formation.
