The galaxy exhibits a disk-like morphology, observed at an edge-on or highly inclined angle with respect to our line of sight. The central region displays a concentrated bulge that appears moderate in size. Faint traces of spiral arm structure are potentially present, though their visibility is limited by the viewing angle. There is a hint of a possible bar feature in the central region, extending along the major axis. The galaxy's overall color profile suggests a relatively evolved stellar population, with a greater concentration of older stars in the bulge. The outer regions of the disk appear less defined, exhibiting a gradual decrease in luminosity, and have a hint of bluer color. The overall shape is elongated and thin. No indications of ongoing major merging events are readily apparent, though minor disturbances in the disk’s structure might be present.
