The galaxy presents as a centrally concentrated object, displaying a smooth, oval-shaped morphology. The core exhibits a bright, yellowish-white luminosity, suggestive of a substantial population of older stars. Moving outwards, the light gradually fades into a more diffuse, greenish-yellow disk or halo. There's a subtle hint of a more flattened structure, though without distinct spiral arms, and no strong indications of active star formation regions are immediately visible. There are also no signs of tidal tails or major disturbances from any significant merger events. There might be a very faint outer disk or halo.
