The galaxy presents a flattened, disk-like structure, indicating it is likely a spiral or lenticular galaxy. It appears to be tilted relative to our line of sight, showing a clear major and minor axis. The central region displays a concentrated bulge, exhibiting a yellowish hue, potentially indicative of an older stellar population. Surrounding the bulge, a fainter disk is visible, with hints of spiral arm structure. The disk displays a bluer color compared to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. There is some indication of dust lanes within the disk, appearing as slightly darker regions against the brighter stellar light. The outer regions of the disk fade gradually into the background. The overall morphology suggests a fairly evolved galaxy.
