The galaxy presents as a somewhat smooth and centrally concentrated object. Its overall shape is more elliptical than circular, but not highly elongated. There's a suggestion of a subtle disk-like structure, though it is not prominent. The galaxy appears to be undergoing only minor disturbances if any at all. A slight asymmetry in the distribution of light is visible within the main body. The color gradient suggests a population of older stars dominating the central region, with hints of bluer, possibly younger, stellar populations towards the periphery. Redder regions may indicate areas of dust obscuration or older stellar populations. Overall, the galaxy appears to be a fairly massive system with a modest star formation rate.
