The galaxy presents an elongated, lenticular morphology, viewed at a nearly edge-on orientation. The central bulge appears luminous and exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the disk shows a bluer tint, possibly indicating regions of more recent star formation, though the image resolution is not high enough to resolve individual star-forming regions. The outer edges of the disk appear somewhat diffuse, fading into the background sky. There is no clear evidence of strong spiral arm structure or a prominent dust lane. Overall, the galaxy appears relatively smooth in texture, with no major signs of ongoing mergers or significant tidal disturbances. It seems to have a fairly high mass, suggesting it is a fairly large galaxy. Its mass suggests it may have a slower specific star formation rate, indicating a less active galaxy. 
