The galaxy presents as a slightly elliptical, disk-like structure, viewed at an oblique angle. The central region exhibits a bright, concentrated bulge or core, suggesting a significant concentration of older stellar populations. Moving outward from the center, the light distribution gradually diminishes, transitioning into a fainter, more diffuse disk component. The disk appears relatively smooth, with only subtle variations in brightness, and no evidence of prominent spiral arms or distinct dust lanes are visible. There appears to be no apparent ongoing major merging activity or significant tidal distortions, although a minor disturbance can not be ruled out due to the lack of higher resolution images. Overall, the galaxy appears relatively undisturbed.
