The galaxy presents as a relatively smooth, centralized light distribution with a dominant spherical or elliptical morphology. There is little evidence of distinct spiral arms or a prominent disk structure. The central region exhibits a bright, concentrated glow, suggesting a substantial concentration of stars and potentially an active galactic nucleus. The light from the galaxy seems fairly uniform in color, with subtle gradations from a blueish-white core to a warmer, yellowish outer halo. This color suggests a stellar population with a wide range of ages, but the relative brightness indicates that the light is dominated by blue, younger stars. There is a possible faint disk-like structure extending away from the central region, but it's poorly defined. There is a subtle asymmetry in the galaxy's shape, hinting at the possibility of past interactions or mergers, or internal processes such as tidal disturbances.
