The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is yellow in color, indicative of an older stellar population. The galaxy's light profile seems largely uniform, with a gradual decrease in brightness moving outward from the core, although the outer regions are faint. 

There is some indication of a slight asymmetry or possible minor disturbance in the galaxy's morphology. It is possible there is some level of merging or tidal interaction occurring. Overall, the galaxy appears as an early-type system with a dominant spheroid component.
