The galaxy presents as a centrally concentrated, smooth light distribution. It appears elliptical in shape, with a slightly elongated profile. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The outer regions display a gradual decrease in surface brightness with hints of faint blue light, potentially indicating pockets of ongoing star formation. Overall, the galaxy's structure is largely undisturbed, showing no obvious signs of major merger activity, though subtle irregularities in the outer isophotes might suggest minor interactions in its past.
