The observed galaxy presents as a well-defined spiral structure, with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Two distinct spiral arms emanate from the central bulge, demonstrating a fairly organized structure. These arms display a predominantly bluish tint, indicative of active star formation regions and a younger stellar population. The winding of the spiral arms appears to be intermediate, showing neither tightly wound nor loosely defined arms. Evidence suggests a barred structure is present within the central region of the galaxy, although it appears partially obscured by the bulge. There's no apparent sign of significant tidal disruption or major merger activity, with no extended or irregular features to suggest a recent interaction with another galaxy. The estimated size of the galaxy is considerable, indicating a substantial stellar mass. The overall appearance suggests a relatively undisturbed spiral galaxy undergoing normal star formation within its spiral arms.