The galaxy presents a primarily smooth morphology. There appears to be a high degree of rotational symmetry. The galaxy's light is concentrated centrally, with intensity decreasing radially. The core exhibits a yellow-white hue, suggesting a population of older stars. Progressing outward, the color profile transitions into a blue-green tinge. There is no apparent disruption to the galaxy's structure, suggesting a lack of recent major merger events. The galaxy could be classified as an elliptical galaxy given its shape. The half-light radius appears rather small. Star formation is quite low.
