The galaxy presents as a largely homogenous, smooth elliptical structure. The light profile appears concentrated towards the center, gradually decreasing outwards. There is a slight elongation, but it is mostly spheroidal in shape. No prominent spiral arms, dust lanes, or active galactic nuclei are apparent within the limitations of the image resolution. A very faint bluish halo may be present, but the low-resolution and potential image artifacts make it difficult to confirm. The overall color is moderately red, which could indicate an older stellar population.
