The galaxy appears as a relatively compact, smoothed structure with a discernible but subtle disk. The morphology seems to be largely dominated by the bulge component, which gives it a mostly elliptical shape. The galaxy exhibits a smooth texture overall, indicating a relatively evolved stellar population. The color gradient within the galaxy shows a shift from a yellower central region to a slightly bluer outer halo. This color variation could imply a difference in stellar age and composition, with older, redder stars concentrated toward the galactic center and younger, bluer stars populating the outer regions. There is no apparent indication of strong tidal disturbances or ongoing major merger events.
