The galaxy presents as a spiral type, viewed at a moderate inclination angle. The disk exhibits defined spiral arms, although their structure is somewhat flocculent rather than grand design. These arms appear slightly distorted or uneven in their distribution. There is a clear central bulge, which dominates the luminosity of the inner region. The bulge appears more prominent and concentrated than the outer disk. The color gradient indicates that the bulge is comprised of older stars with a yellowish hue. The disk is bluer, especially along the spiral arms, which suggests ongoing star formation. There is no obvious bar structure, but there is also no evidence of interaction with other galaxies or major mergers, although some minor disturbances or asymmetries are possible. The overall structure points toward a mature spiral galaxy with moderate star formation activity.
