The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light profile appears to be relatively uniform, lacking any prominent spiral arms or significant dust lanes. The color gradient suggests a possible radial change in stellar population, with a slightly bluer hue towards the outer regions and a yellower tint near the core. There is a subtle asymmetry in the light distribution, indicating a possible minor interaction. No obvious signs of a major merger event, such as tidal tails or strong distortions, are apparent in the image.
