The observed galaxy presents as a disk galaxy, viewed nearly edge-on. The primary axis of the disk is oriented horizontally across the image. There is a prominent dust lane bisecting the galaxy along its mid-plane, obscuring the light from stars and nebulae located behind it. The bulge appears somewhat boxy in shape and contributes significantly to the overall luminosity profile, although is not substantially dominant. The disk exhibits a complex morphology with some evidence of spiral arm structure visible despite the edge-on perspective. The outer regions of the disk appear fainter and somewhat diffuse, hinting at a gradual decline in stellar density. Color gradients are observed with bluer hues generally noted in the outer regions and along the edges of the dust lane, suggestive of ongoing star formation activity in these areas. The overall system appears relatively undisturbed, with no clear signs of a recent major merger or strong tidal interactions. The average SFR appears low.
