The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, appearing cigar-shaped. There's a noticeable central bulge with concentrated luminosity. The color profile suggests a population of older stars, with a bias towards redder wavelengths in the outer regions and a somewhat bluer core. No prominent spiral arms or distinct dust lanes are visible within the galaxy's structure. There are no signs of any major mergers or tidal disturbances in the surrounding galactic halo.
