The galaxy presents as a moderately bright, elliptical form. The light profile is smooth, with no discernible spiral arms or bar structure. The central bulge is concentrated and exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the galaxy appears less concentrated, displaying a diffuse bluish halo, possibly indicating some presence of younger, hotter stars and ongoing or recent star formation. The overall shape is elongated, appearing cigar-shaped, and shows no obvious signs of major mergers or significant tidal disturbances. There is slight asymmetry to the galactic disk, indicating either a minor interaction or uneven distribution of matter. The galaxy is of intermediate size, neither exceptionally large nor particularly small.