The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The overall color appears to be yellowish-orange, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are readily apparent. There is a slight elongation to its shape; it is not perfectly spherical, leaning towards a more cigar-like appearance. The galaxy seems relatively isolated, displaying no signs of any major ongoing merger activity, although there might be a hint of a minor disturbance in the outer regions based on slightly uneven light distribution. Star formation appears to be generally suppressed. The galaxy is approximately 9.5 kpc in radius.
