The galaxy presents as a centrally concentrated, smooth object with a roughly elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting a population of older stars and potentially lower levels of current star formation compared to bluer galaxies. There is a noticeable radial decrease in surface brightness from the core outward. The galaxy appears relatively undisturbed, lacking prominent spiral arms or tidal features indicative of recent major mergers, however there seems to be a minor disturbance in the outer edges of the galaxy. Its overall shape can be described as moderately elliptical, with an intermediate axis ratio. Faint bluer light is observed in the surrounding halo.
