The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, deviating slightly from perfect circularity. A central bulge is discernable, though not sharply defined, exhibiting a brighter, more intense luminosity compared to the outer regions. A faint, diffuse halo surrounds the central structure, gradually fading into the background sky. The galaxy exhibits a subtle color gradient, with the core appearing slightly bluer than the outer regions, hinting at younger stellar populations in the central regions. There is no clear evidence of spiral arms or significant dust lanes. No ongoing major merger is visibly apparent, though minor morphological disturbances cannot be ruled out, although there is no obvious signature of strong tidal interactions or ongoing starburst activity.
