The galaxy appears as a somewhat amorphous, elliptical structure. The central region exhibits a high degree of luminosity, suggesting a concentrated population of stars, or potentially an active galactic nucleus. Moving outward from the core, the light gradually diminishes, with no distinct spiral arm structures apparent. The edges are fuzzy and ill-defined, blending smoothly into the surrounding background sky. There are hints of slight disturbances or asymmetries in the outer regions, which could be indicative of a past or ongoing merger event, although the dominant impression is one of relatively smooth distribution of stellar material. The overall color profile suggests a mix of stellar populations, with the core leaning towards a slightly older, redder population, while the fainter outer regions possibly contain some bluer, younger stars.
