The galaxy presents as a diffuse, generally smooth, yet somewhat complex system. There appears to be a central, brighter region indicative of a galactic bulge, surrounded by a more extended, fainter halo. Color gradients are present, shifting from bluer hues in the central region to redder tones in the outer regions. This could be indicative of differing stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars dominating the halo. The overall morphology suggests a relatively evolved system, potentially an elliptical or lenticular galaxy. However, there seems to be a small disk like structure on the bottom right side of the object, which may indicate a disk component within the galaxy. There is also a minor disturbance on the top right region of the galaxy in the form of a second region of light. A small tidal feature may be present, or there may be a companion galaxy. Further spectroscopic analysis would be necessary to determine the nature of the stellar populations and dynamics within this system, as well as the cause of the minor disturbance.
