The galaxy appears to be an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The central region presents a bright, yellowish hue, potentially indicating an older stellar population and a relatively low rate of ongoing star formation. Moving outwards from the center, the light fades gradually, and the color shifts toward slightly bluer tones, possibly signaling the presence of younger stars in the outer regions, although these populations are less prominent. The overall shape is nearly circular, with no obvious signs of spiral arms or a bar structure. There are no visual indications of significant tidal disturbances or interactions with other galaxies. Based on these observations, the galaxy can be characterized as a relatively massive, early-type galaxy with a relatively smooth structure.
