The observed galaxy presents a clear disk morphology, viewed at an angle. Faint spiral arms are visible. The galaxy's light profile exhibits a centrally concentrated bulge. The bulge size can be described as relatively small in comparison to the disk. The central region presents a yellowish hue, which likely indicates a population of older stars. The outer disk demonstrates a bluer color, indicating a younger stellar population and ongoing star formation. There is no sign of a bar structure in the central region. No signs of a major merger are visible, but a faint disturbance cannot be ruled out, particularly in the extended disk. The galaxy has a mass range of 10^10.8 to 10^10.9 solar masses and a low star formation rate. The estimated size of this galaxy is approximately 4.5 kiloparsecs.
