The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a bright, yellowish hue, suggesting a concentration of older stellar populations. Moving outward from the core, the color gradually shifts towards a bluer tint, indicating the presence of younger, hotter stars. There is a subtle suggestion of a disk-like component. The galaxy lacks any pronounced spiral arms or irregular features, indicating it is not actively undergoing a major merger or starburst event. Some minor disturbance is possible. The overall morphology suggests an elliptical or lenticular classification, observed at an oblique angle.
