The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. Fainter, bluer light emanates from the disk, suggesting the presence of younger stars and ongoing star formation. The disk structure appears relatively smooth, with little evidence of strong spiral arms or distinct features. There are subtle asymmetries or minor disturbances in the disk's morphology, but not enough to suggest a major ongoing merger. Overall, the galaxy appears to be a relatively quiescent, late-type spiral galaxy with moderate star formation activity. The size appears to be relatively compact. The disk is thin and elongated.
