The galaxy presents as a moderately luminous object, exhibiting a concentrated central bulge of primarily yellowish-orange hue. The overall morphology appears generally smooth, with no immediately discernible spiral arm structures or significant dust lane obstructions. The shape is approximately elliptical, tending towards a flattened spheroid. Subtle color variations are noted across the galaxy's body, with slightly bluer tinges observed at the outer edges. The central bulge is the brightest region, with the luminosity decreasing gradually toward the periphery. There is no apparent strong active galactic nucleus. No obvious signs of recent major merger events or tidal disturbances can be observed. Based on the color profile, the galaxy likely contains an older stellar population in the central regions, with a possibility of ongoing or recent star formation occurring within the disk.
