The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology. There is a concentration of light towards the center, indicating a prominent galactic bulge. The color profile shows a redder hue in the central regions, which may suggest an older stellar population. Moving outward from the core, the light becomes fainter and slightly bluer, indicative of younger, hotter stars in the outer regions or potentially some ongoing star formation. The overall shape is somewhat elongated rather than perfectly circular, and there's no apparent spiral arm structure or dust lanes visible in this image. There may be minor disturbances in the outer regions of the galaxy, although they do not appear to be related to an ongoing major merger event. The galaxy exhibits a definite core with a gradual decrease in luminosity toward its edges.
