The galaxy presents as a disk galaxy, observed at a moderate angle to our line of sight. The central bulge appears prominent and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions are distributed throughout the disk, indicative of more recent star formation. The galaxy exhibits some signs of morphological disturbance, with slight asymmetries and some fainter patches, possibly due to minor tidal interactions or internal processes. There may be slight indications of some spiral structure, though it is faint and not strongly defined.
