The galaxy presents as a relatively compact, disk-shaped structure. Its disk appears to be oriented nearly edge-on with respect to the observer's line of sight. The central bulge is not obviously prominent, if present at all. The luminosity profile appears smooth, lacking distinct features such as spiral arms or star-forming knots. Color gradients are evident; the edges of the disk exhibit a bluer hue, possibly indicative of younger stellar populations or ongoing star formation, whereas the central regions appear redder. Some asymmetry is observed in the disk, with one side appearing slightly more extended or disrupted than the other. There may be some evidence of minor tidal disturbances or interactions, although no clear companion galaxies or tidal tails are immediately apparent. Overall, the galaxy exhibits characteristics of a relatively quiescent system, with moderate size, and minimal star formation activity.
