The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A central bulge is evident, appearing smoothly rounded and brighter than the surrounding disk. The disk component shows little to no resolved structure, indicating a relatively smooth distribution of stars and dust. The color gradient suggests a possible stellar population difference, with the central bulge exhibiting a yellower hue, indicative of older, redder stars. The outer disk appears slightly bluer, potentially indicating younger, hotter stars and ongoing star formation, but the resolution is insufficient to confirm individual star-forming regions. There is no visual evidence of significant merger activity or tidal disturbances in the immediate vicinity of the galaxy.
