The galaxy presents as an edge-on spiral, with a clearly defined disk oriented at a high inclination relative to our line of sight. The central bulge appears prominent, exhibiting a smooth, yellowish color suggesting an older stellar population. The disk component shows a bluer tint towards the outer edges, possibly indicative of more recent star formation activity. There is a defined dust lane running horizontally across the middle which adds to the redness of the bulge. Overall, there does not seem to be any evidence of active galactic nuclei. There are no other irregularities in the image.