The galaxy appears as an elongated, disk-shaped structure. It is oriented edge-on or nearly edge-on from our perspective. The central bulge is subtle, appearing slightly brighter and more concentrated than the rest of the disk. 

There is evidence of a prominent dust lane bisecting the galaxy, obscuring the light from stars located behind it. The color profile indicates the presence of both older stellar populations exhibiting yellow or reddish hues, especially toward the bulge, and bluer regions indicative of younger stars and ongoing star formation within the disk.

There is an indication of a possible minor tidal disturbance or faint plume emanating from the galaxy, suggesting a recent or ongoing interaction or merger event with a smaller companion galaxy. However, it does not seem to be undergoing a major merging event.
