The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution. The central region appears as a concentrated bulge with a yellowish hue, potentially indicating a population of older stars. Moving outwards, the galaxy has a more diffuse appearance, exhibiting a subtle gradient in color, shifting towards a slightly bluer tint in the outer regions, suggesting the presence of a younger stellar population within the disk. There are no immediately obvious signs of strong spiral arms, bars, or active galactic nucleus activity discernible in this image. There is a slight possibility of minor disturbances in the outer disk but it is not conclusive based on the image alone. Overall, the galaxy appears to be in a relatively undisturbed state with a mix of stellar populations present.
