The galaxy presents as a centrally concentrated object. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars or potentially an active galactic nucleus. Moving outward from the core, the light distribution becomes more diffuse. There is a slight elongation in shape, but the galaxy appears mostly spheroidal. There is some indication of disturbed morphology and possible interactions with other galaxies. The outer regions have a fainter, less defined structure, indicating a lower density of stars and gas at larger radii. Some of the light in these areas has a reddish tint.