The galaxy presents as a single, relatively smooth object with a concentrated central bulge or core. Its overall shape is approximately elliptical or spheroidal, with a high degree of symmetry. The color profile appears uniformly yellowish, suggesting a dominant population of older stars. There is no apparent evidence of spiral arms, significant dust lanes, or active star formation regions within the visible light spectrum. No signs of tidal tails, merging, or other disturbances that would indicate recent or ongoing interactions. This suggests the galaxy is likely a well-formed, quiescent system that is not undergoing significant evolutionary changes in its current state.
