The galaxy presents as a moderately bright, elliptical structure. Its core exhibits a high degree of luminosity, suggestive of a concentrated stellar population. Progressing outward from the core, the luminosity decreases smoothly, indicating a gradual falloff in stellar density. The overall color appears somewhat redder in the outer regions compared to the central core, which may signify older stellar populations in the galaxy's halo. There is minimal visual evidence of distinct spiral arms or prominent dust lanes. The galaxy seems relatively undisturbed, with no signs of major tidal distortions or ongoing mergers readily apparent in the image.
