The galaxy appears to be a relatively smooth, elliptical-type galaxy, with an overall rounded morphology. There is a concentration of light towards the center, indicating a prominent bulge. The galaxy displays a color gradient, shifting from a yellower, possibly older stellar population in the core, to slightly bluer, potentially younger stellar populations in the outer regions. There is no clear evidence of a spiral structure or a well-defined disk component from this view. There may be faint irregularities in the outer regions, potentially suggesting minor disturbances, but the overall structure is quite smooth and regular.
