The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical, with a gradual decrease in luminosity extending outwards into a more diffuse halo.  Faint, asymmetric features may suggest a minor tidal interaction or past merger event, however this galaxy is mostly undisturbed. There is a noticeable color gradient, trending from a bluish-white core to a redder periphery. This color variation may indicate a difference in stellar populations, with younger, hotter stars dominating the central region and older, cooler stars populating the outer regions. No distinct spiral arm structures or prominent dust lanes are observed. The galaxy appears relatively compact with an estimated diameter of 4 kiloparsecs, given its distance based on redshift. This is a relatively small mass galaxy, and is in a fairly active stage of star formation.
