The galaxy appears to be an elliptical galaxy, exhibiting a smooth and round morphology. There is a central bulge that is bright and dominant. Faint, diffuse light extends from the central region, gradually fading into the background. No prominent features such as spiral arms or dust lanes are readily apparent. The overall color profile suggests a population of older stars. There are no signs of ongoing major merger activity, although subtle disturbances or tidal features cannot be entirely ruled out given the image resolution.
