The galaxy presents an overall elliptical morphology, elongated along its major axis. There appears to be a prominent central bulge, exhibiting a smooth, concentrated light profile. Surrounding the bulge is a disk component, though it appears relatively disturbed or irregular in structure. Distinct features are visible within the disk, specifically two arcs of red, likely indicating regions of active star formation, potentially triggered by tidal interactions. The overall color profile suggests the presence of both older stellar populations (contributing to the reddish hue of the bulge) and younger, hotter stars (within the blueish arcs). There appears to be minor structural asymmetry, possibly indicative of a past or ongoing merger event or gravitational interaction with another galaxy. The estimated angular size indicates a relatively compact object.
