The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity, surrounded by a luminous halo.

The disk component appears relatively thin and shows evidence of dust lanes, particularly visible as darker bands bisecting the brighter regions of the disk. These lanes suggest obscuration of starlight by interstellar dust.

There is a hint of possible interaction or minor disturbance affecting the structure. A small, asymmetric warping in the disk is observed, with one side appearing slightly distorted. This may be indicative of tidal interaction with a smaller object.

Based on its structure, this galaxy is likely a spiral galaxy, though the details of its spiral arms are obscured by the edge-on viewing angle.
