The galaxy presents a generally smooth morphology, with a dominant central bulge that is more luminous and compact than the surrounding galactic disk. The light distribution appears relatively even and the galaxy presents an elliptical shape. The core is a distinct yellowish-orange color, possibly indicative of an older stellar population, while the outer regions have a slightly bluer hue, suggesting more recent star formation in the disk. There is no clear evidence of spiral arm structure or strong dust lanes within the limits of image resolution. There is no obvious indication of major mergers or significant tidal disturbances impacting the system. 
