The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. It appears largely elliptical, with a high degree of roundness. There's a suggestion of minor internal structure, but no obvious spiral arms or bar features are discernible. The galaxy appears to be a primarily quiescent system with low levels of star formation. The color suggests a higher population of older stars, corresponding to a higher mass. Close inspection does not reveal any signs of major interactions or ongoing mergers, although very subtle disturbances cannot be ruled out at this resolution.
