The galaxy presents as an elongated structure with a primary color gradient shifting from a central bluish-white hue to a reddish tinge at its periphery. The core region exhibits a smooth texture suggesting a high concentration of older stellar populations. Extending outward, a fainter, more diffuse disk component is visible, potentially indicative of ongoing, but not extremely vigorous, star formation. The overall symmetry is slightly perturbed, possibly hinting at minor gravitational interactions or internal disturbances. There isn't a clear spiral arm structure, but there appears to be a disk feature. The galaxy lacks strong tidal tails or other extreme morphological irregularities associated with major mergers.
