The galaxy presents as a single, relatively smooth concentration of light. It exhibits a spheroidal morphology, with a high degree of roundness, and an overall homogenous appearance. There is a noticeable lack of distinct features such as spiral arms or a prominent central bulge, suggesting a classification toward the elliptical end of the Hubble sequence. The color appears to be yellowish, which suggests an older stellar population and limited ongoing star formation. There are no visible signs of recent or ongoing major mergers or tidal disturbances in the immediate vicinity. The galaxy's light distribution declines smoothly and evenly from the center outwards.
