The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears to be trending towards the redder end of the spectrum, with a bright yellowish core that fades into less defined outer regions. The light distribution suggests a spheroidal or elliptical morphology, showing no obvious spiral arm structures or strong disk component. While generally smooth, some very faint asymmetries or minor disturbances might be present upon closer inspection, but the resolution limits definitive identification. The outer edges appear diffuse, gradually blending into the background sky. No signs of a recent major merger event are evident.
