The galaxy presents as a moderately luminous object exhibiting a smooth, elliptical morphology. A central bulge dominates the structure, displaying a concentrated, yellowish-white hue, indicative of an older stellar population. Extending outward from the core, a diffuse, bluish halo is observed, suggesting the presence of some younger stars and ongoing, albeit low-level, star formation within the galactic outskirts. There are no prominent spiral arms or bar structures visible. There may be slight irregularities in the outer structure, but overall the galaxy appears relatively undisturbed.
