The galaxy presents a generally smooth and elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The galaxy displays a subtle color gradient, transitioning from a slightly bluer hue in some regions to a redder hue in others. There is no clear spiral arm structure or strong evidence of a prominent disk component visible in this image. However, there appears to be some subtle disturbance in the smoothness, and the galaxy might be a merging galaxy. The overall shape is predominantly round, although some elongation is present.
