The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. There is a clear lack of discernible spiral arm structure. The color profile suggests a population of older stars, with a dominant yellowish-red hue in the central regions, transitioning to a bluer tinge at the outer edges. The galaxy appears to be generally undisturbed, exhibiting no signs of major mergers or tidal interactions. There may be some low-level star formation occurring, contributing to the slight bluing observed peripherally. The overall impression is that of a mature, quiescent galaxy.
