The galaxy presents as a somewhat elliptical, though not perfectly spherical, luminous object. A dominant central bulge is apparent, exhibiting a smooth morphology with no immediately discernible dust lanes or spiral arm structures. The light distribution appears concentrated towards the center, suggesting a relatively high degree of central mass concentration. Its color is generally yellowish-orange, possibly indicative of an older stellar population with a relatively low rate of on-going star formation. Some minor disturbances are visible in the morphology, but these do not significantly disrupt the overall smooth appearance.
