The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with the majority of its light emanating from a bright, yellowish core. There is a gradual decrease in surface brightness moving outward from the center, transitioning to a fainter, more diffuse halo. The overall color profile suggests a population of older stars, contributing to the galaxy's yellowish-red hue. No distinct spiral arms or prominent dust lanes are discernible. There may be some minor disturbances to the galaxy's smooth structure, but the bulk of the light appears even. There appears to be an absence of recent star formation.
