The galaxy presents as a single, relatively smooth object with a concentrated central region. Its morphology appears largely spheroidal, exhibiting a high degree of circular symmetry. There is little evidence of spiral arms or a defined disk structure. The galaxy's color profile suggests a predominantly older stellar population. The light is redder in the core, transitioning toward slightly bluer hues in the outer regions. There is no apparent dust lane. No major mergers or tidal tails are visible.
