The galaxy presents as a centrally concentrated, elliptical-like system, exhibiting a smooth, featureless morphology in the visible light spectrum. The luminosity profile appears to increase monotonically towards the core. The central region displays a yellowish hue, potentially indicative of an older stellar population, suggesting a reduced rate of ongoing star formation. There appears to be no evidence of spiral arms or a prominent galactic disk. The galaxy appears relatively isolated, with no signs of major mergers or significant tidal disturbances in its immediate vicinity, although minor disturbances cannot be ruled out. Its rounded shape suggests an advanced stage in its morphological evolution.
