The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, appearing as a bright, yellowish core. Moving outward, the light gradually diminishes, creating a diffuse halo. There is a subtle elongation, though the overall shape approximates a spheroid. No distinct spiral arms or prominent dust lanes are discernible. The color suggests a stellar population that is largely evolved with moderate star formation activity. There is no visible evidence of ongoing mergers or major tidal disturbances impacting its structure. The galaxy’s structure appears undisturbed and in a relatively relaxed state.
