The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, concentrated morphology. It displays a noticeable elongation, appearing cigar-shaped. There is little discernible dust or distinct spiral arm structure visible. The galaxy appears relatively undisturbed, without any major signs of tidal interactions or ongoing mergers. It has a strong central bulge with a gradual decrease in luminosity towards the outer edges. The color profile suggests an older stellar population, biased towards redder wavelengths. Star formation appears to be minimal.
