The galaxy appears as an elongated, disk-like structure, observed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. Extending outward from the bulge is a fainter, somewhat diffuse disk. There is evidence of possible disturbances in the disk, which could be indicative of minor tidal interactions or mergers. The galaxy's overall color suggests a moderate level of on-going star formation, although the bulk of its stellar mass likely resides within the bulge.
