The galaxy appears to be a relatively smooth, elliptical or lenticular system. The central bulge is prominent and shows a concentration of light, suggesting a high stellar density. There is a noticeable absence of strong spiral arm structures or prominent dust lanes. The overall color is yellowish, implying an older stellar population with a low rate of ongoing star formation. The galaxy exhibits a somewhat rounded morphology. There is a hint of possible minor tidal disturbance in the form of faint asymmetry, but the overall impression is that of a relatively relaxed, isolated system.
