The galaxy appears as a single, centrally condensed object with a smooth, relatively featureless profile, lacking prominent spiral arms or a well-defined disk. The central region exhibits a bright, concentrated luminosity, while the outer regions gradually fade into the background. The color profile suggests a population of older stars, with a dominant yellowish-red hue. The light distribution is roughly spherical in shape, with no obvious elongation or tidal features indicative of strong gravitational interactions. A slight asymmetry can be seen, suggestive of possible past interactions or internal dynamical processes. The galaxy is relatively compact in size.
