The galaxy presents as a generally smooth, elliptical-like structure with a bright, concentrated central bulge. The main body exhibits a yellowish-orange hue, suggesting an older stellar population. There is some elongation present, it is more "in between" round and cigar-shaped. Little indication of spiral arms or significant dust lanes are seen. A slight asymmetry is observed in the outer regions. The overall impression is of a galaxy undergoing passive evolution, with low rates of star formation. No sign of major merger event.
