The galaxy presents as a largely smooth, elliptical-like structure, with a concentrated central bulge that appears quite luminous. The color appears to be somewhat redder, with slight variations in intensity across the main body. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. Based on the smooth appearance and color, it is likely this galaxy consists predominantly of older stellar populations, with relatively low ongoing star formation. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal distortions, although subtle irregularities may be present. The galaxy possesses an estimated physical size of several kiloparsecs. Overall, the object appears to be a reasonably massive galaxy, consistent with a mature system.
