This galaxy appears to be a spiral galaxy observed nearly edge-on. A prominent bulge is visible, exhibiting a yellowish hue that indicates an older stellar population. The disk is characterized by a bluer color suggesting ongoing star formation. There are no clear signs of distinct spiral arm structure, and no evidence of a major merger is readily apparent. The bulge appears to be slightly rounded, but is difficult to further characterize given the lack of resolution in the image. The galaxy seems relatively undisturbed, lacking any obvious tidal features or asymmetries, though minor disturbances or a past merger cannot be entirely ruled out at this resolution. The galaxy is relatively compact, with a moderately bright core.