The galaxy presents as a moderately bright, elliptical-shaped structure. The central bulge exhibits a concentrated, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the color transitions to a bluer, more diffuse region. The overall morphology indicates a galaxy that is neither perfectly round nor highly elongated. There are no readily apparent spiral arms or significant dust lanes visible in this image. The edges of the galaxy fade gradually into the background, indicating a smooth decline in stellar density. There are no significant features to suggest an ongoing major merger event, though some minor distortions could be present within the extended halo. The galaxy appears relatively smooth and featureless.
