The galaxy presents as a generally smooth, elliptical-like structure. Its core is a bright, concentrated yellowish-white, suggesting a significant population of older stars. The overall shape appears somewhat elongated, neither perfectly spherical nor a highly flattened disk, with a moderate axial ratio. Faint reddish hues surround the central region, possibly indicating regions of dust or older stellar populations. There is no apparent spiral arm structure or evidence of significant recent star formation in the outer regions of the galaxy. It exhibits no clear signs of ongoing major mergers or tidal disturbances.
