The galaxy presents a predominantly smooth, elliptical morphology. It appears to be moderately inclined relative to our line of sight, exhibiting an elongated shape. The central region displays a high concentration of light, suggesting a prominent galactic nucleus. The light distribution becomes more diffuse towards the outer regions of the galaxy. There appears to be a slight disturbance or asymmetry in the galaxy's structure, possibly indicating a minor interaction with another galaxy, or an internal asymmetrical phenomena. The color gradient shows a shift from yellow-orange in the center to a more blue hue in the outer regions. This color distribution indicates a potential variation in stellar populations, with older, redder stars concentrated in the galactic bulge, and a relatively younger, bluer stellar population residing in the outer regions.
