The galaxy presents as a relatively compact and centrally concentrated object. Its overall morphology appears largely smooth, with a noticeable radial gradient in luminosity. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, the galaxy displays a gradual color shift towards a slightly bluer and less intense glow, possibly indicating a younger stellar population further from the galactic nucleus, though this difference is subtle. There are no readily discernible spiral arms, bar structures, or other distinct features typically associated with actively star-forming galaxies, though the resolution is limited. The galaxy's overall shape approximates a slightly elongated spheroid, with no obvious signs of tidal disruption or ongoing major mergers. The outer edges fade smoothly into the background, indicating a well-defined boundary, but lacking significant extended halos or plumes.
