This galaxy presents as an edge-on spiral, exhibiting a prominent disk oriented nearly perpendicular to our line of sight. The dust lane is heavily obscured. The central bulge appears bright and concentrated, displaying a spheroidal morphology, consistent with a classification as a late-type galaxy. The galaxy exhibits a notable disk, showing internal structure. There is minor disturbance. No apparent tidal features or signs of interaction with other galaxies are evident. The color profile suggests an evolved stellar population. Overall, this appears to be a substantial galaxy.
