The galaxy presents as a moderately luminous object, exhibiting a notable degree of central concentration. The morphology appears to be that of a disk galaxy seen at a significant inclination. A central bulge is discernible, elongated along the same axis as the overall galaxy. There is evidence of some spiral arm structure, although it appears relatively tightly wound and somewhat flocculent. The color profile suggests the presence of both older stellar populations, contributing to the central bulge and disk, as well as younger, bluer stars potentially within the spiral arms. Some degree of asymmetry or minor disturbance is also suggested, though a merger is unlikely. The galaxy is relatively compact. The rate of star formation is low. The galaxy is thought to be a mass around 10^9 solar masses.
