This galaxy presents as a spiral with a prominent disk structure. The spiral arms appear well-defined, exhibiting a clear pattern of winding, seemingly of medium tightness. Two distinct arms are visible, extending from the central bulge. A bar feature seems to traverse the central region of the galaxy, with some indication of a strong component. The central bulge appears moderate in size, exhibiting a yellowish hue, possibly indicative of an older stellar population. The disk component shows evidence of ongoing star formation, particularly within the spiral arms, exhibiting a bluer color. There are no apparent signs of major mergers. Minor distortions are visible, particularly near the outer regions of the disk, suggesting some interaction. The galaxy is inclined at an angle that allows the disk structure and arm morphology to be observed clearly. Overall, it displays characteristics consistent with a spiral galaxy, exhibiting a combination of features suggestive of both past and current activity.
