The galaxy presents as an elongated, disk-like structure with a relatively smooth overall appearance. It appears to have a central bulge that is more luminous and concentrated than the rest of the disk, with a yellowish hue. The disk itself exhibits a bluer color. There seems to be a hint of a feature or possible companion located near one end of the disk, appearing as a small, reddish, and slightly distinct concentration of light, indicating a possible minor interaction or ongoing accretion event. The majority of the galaxy exhibits a relatively smooth profile, suggesting either a lack of significant ongoing star formation within the primary disk structure or the presence of a dominant older stellar population throughout the region. The general shape is suggestive of an intermediate disk galaxy type, possibly undergoing some form of disturbance.
