The galaxy presents as an elliptical or lenticular type system, characterized by a smooth, largely featureless light distribution. The overall shape appears moderately elongated, displaying a deviation from perfect circularity. There is a suggestion of a central bulge, though it is not sharply defined. The color appears to be on the redder end of the spectrum. While no distinct spiral arms or prominent dust lanes are visible, subtle variations in surface brightness may indicate underlying structural elements. No obvious signs of tidal interactions or major mergers are apparent, though subtle disturbances could be present at a level below the image resolution. The system appears relatively isolated in this field of view.
