The galaxy presents as a moderately luminous, relatively smooth object. Its morphology appears largely elliptical or lenticular, displaying a diffuse, spheroidal structure with minimal discernible substructure. The color profile suggests a population dominated by older stars, evidenced by the redder central bulge region. There is evidence of a faint, extended halo, exhibiting a bluer color compared to the core, indicating the presence of younger stellar populations or a low level of ongoing star formation, although very quiescent overall. No significant tidal features or signs of recent major mergers are apparent, suggesting a dynamically relaxed system. There may be a slight deviation from perfect ellipticity, but without higher resolution imaging it is difficult to characterize the shape further.
