The galaxy presents a moderately concentrated, elliptical morphology. The core exhibits a strong, yellowish-orange luminosity, suggesting a significant population of older stars and potentially dust obscuration. Moving outward from the core, the light gradually diminishes, indicative of a decreasing stellar density. There appears to be a very faint disk-like structure, with a small, possibly tidal feature extending from one side. While the galaxy's overall form is smooth, there is some slight irregularity in its outer regions, possibly due to a minor disturbance or past merger event. Overall, this appears to be a relatively massive galaxy undergoing a low level of star formation.
