The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The isophotes are closely spaced, indicating a centrally concentrated luminosity profile. The overall shape is more rounded than cigar-shaped. There is a slight visual asymmetry but no significant signs of major merging or tidal disturbances. Faint extensions or a very subtle disk-like structure appear to be present. The light is fairly smooth with subtle color variations across the galaxy. It appears to be relatively inactive in terms of current star formation. The galaxy is generally isolated.
