The galaxy presents as a centrally concentrated object, appearing largely smooth with a notable lack of distinct spiral arms or a prominent bar structure. It exhibits a relatively elliptical morphology, leaning towards a slightly rounded shape rather than an elongated or cigar-shaped form. The color profile suggests a population of older stars, as evidenced by the reddish-yellow hue dominating the central bulge. The outer regions display a bluer tint, potentially indicating the presence of younger stellar populations. While the galaxy appears generally undisturbed, a slight asymmetry in its outer halo suggests a possible history of minor interaction or tidal disturbance.
