The galaxy presents as a moderately luminous, relatively compact system. It exhibits a generally smooth morphology with a high degree of central concentration. The light distribution appears largely elliptical, with a slight deviation towards a more spheroidal shape. There is no strong evidence of spiral arm structure or a prominent disk component. The color profile indicates a dominant population of older stars, particularly towards the central regions, with hints of bluer, potentially younger stars in the outer areas. No obvious signs of active galactic nuclei activity or significant ongoing mergers are apparent. There may be some minor disturbances in the outer region, but this is not definitive.
