The galaxy presents a generally smooth, elliptical morphology with a dominant, centrally concentrated bulge. The light distribution appears to be relatively uniform without prominent spiral arms or significant substructure. The color gradient suggests a higher concentration of older stellar populations, particularly towards the galaxy's core, indicating little active star formation. The light is mainly comprised of redder wavelengths, hinting at a population of evolved stars. No dust lanes or significant regions of blue light indicative of young stars and active star formation are immediately apparent. The overall appearance suggests an evolved galaxy likely undergoing passive evolution. Evidence of past or ongoing interactions seems minimal.