This galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a higher surface brightness, suggesting a concentrated stellar population or potentially an active galactic nucleus. The overall color appears slightly redder, indicative of an older stellar population with relatively little ongoing star formation. There is a subtle elongation in the galaxy's shape, with the light distribution appearing somewhat cigar-shaped. No distinct spiral arms or prominent dust lanes are discernible. The galaxy does not display any obvious signs of tidal disturbances or interactions with other galaxies. The structure appears largely undisturbed and relaxed, which could mean it has undergone mergers in the past but has had time to fully equalize. 
