The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a concentrated central bulge. There is a slight elongation. The light distribution appears fairly uniform, with a color profile trending towards the redder end of the spectrum, indicating a population of older stars. No distinct spiral arms or dust lanes are discernible. There is a slight suggestion of minor tidal disturbance or interaction with a very faint object to the right, but no major merger is immediately evident. The galaxy exhibits a fairly high degree of central concentration.
