The galaxy presents as an elongated, elliptical structure. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. The light profile appears relatively smooth, with a gradual decrease in intensity from the core outwards. The galaxy's color is predominantly yellowish-orange, indicative of an older stellar population. Faint bluish features can be observed towards the periphery, possibly signifying regions of more recent star formation. There is an indication of a possible minor gravitational disturbance that is close by and may be interacting with the larger galaxy. The high roundness ratio also suggests a slight flattening or departure from a perfect sphere.
