This galaxy appears to be an edge-on spiral. A prominent central bulge is visible, exhibiting a reddish-orange hue which suggests an older stellar population within the bulge. The surrounding disk presents a bluer tint toward the outer edges, potentially indicating ongoing star formation. The dust lane along the central plane of the disk is not clearly defined, but there may be minimal disturbances or minor interaction with other objects, as there is no indication of tidal tails or significantly warped disk structure visible in the image. The bulge appears to be roughly rounded, with a slightly brighter center. Overall, the galaxy appears to be relatively undisturbed.
