The galaxy exhibits a predominantly smooth morphology, suggestive of an elliptical or lenticular type. It appears largely featureless in this image, with a high degree of central concentration. The light profile is relatively symmetrical. There is no obvious evidence of spiral arms or a prominent disk structure. The core of the galaxy presents a yellowish hue, potentially indicating an older stellar population or a significant dust component. The outer regions display a slight blueish tint, possibly resulting from younger stars. No obvious signs of ongoing major mergers or tidal disturbances are visible, but subtle minor disturbances cannot be ruled out at this resolution. The overall shape is close to round.
