The galaxy presents as a flattened, elliptical structure with a discernible central bulge. A smooth, diffuse halo surrounds the bulge, exhibiting a gradual decline in luminosity towards the outer regions. The galaxy appears to be inclined relative to our line of sight, as its shape is elongated rather than circular. A hint of spiral structure is present, though not clearly defined; the arms are tightly wound. The overall color profile suggests the presence of both older stellar populations within the bulge, indicated by the yellower hue, and younger, bluer stars potentially contributing to the faint spiral arms within the disk. There is little evidence of significant dust lanes or intense star formation regions. The galaxy appears relatively undisturbed, exhibiting no prominent signs of tidal interactions or major mergers.
