The galaxy presents as a primarily edge-on spiral type, exhibiting a well-defined central bulge that appears yellow, indicating an older stellar population. Extending from the bulge, a faint and blue-tinged disk structure is visible, suggestive of ongoing star formation. The disk appears somewhat disrupted, with some asymmetry. A notable dust lane is likely present but is difficult to distinguish given the image resolution. The galaxy does not appear to be isolated, with hints of tidal features and disturbance in the outer regions of the disk, possibly indicating past or ongoing interactions.
