The galaxy presents as a somewhat inclined disk galaxy. It is likely a spiral galaxy, but no spiral arms are clearly resolved in the available image. The central bulge appears prominent and has a yellowish hue, suggesting an older stellar population with a relative absence of ongoing star formation. A relatively smooth disk surrounds the bulge, exhibiting a bluer color compared to the bulge. This suggests the presence of younger, hotter stars and some ongoing star formation within the disk. The galaxy appears relatively undisturbed, showing no prominent signs of a recent major merger or tidal interactions. There are indications of potential minor disturbances in the disk morphology, but without higher resolution imaging, these are difficult to confirm.
