The galaxy presents a generally elliptical morphology. It appears relatively smooth in texture, with no obvious spiral arms or prominent dust lanes visible in this image. There is a concentrated central bulge of light. The galaxy displays a moderate ellipticity, appearing somewhat flattened. The light distribution becomes more diffuse toward the outer regions of the galaxy, suggesting a gradual decrease in stellar density with increasing radial distance from the center. Color gradients are subtle but present; the central region shows a slightly more yellow-orange hue, while the outer regions trend towards a redder color, potentially indicating a higher proportion of older stellar populations in the outskirts. There are no obvious signs of recent major mergers or significant tidal disturbances.