The galaxy appears as a centrally concentrated, generally smooth object. The core exhibits a bright, somewhat diffuse glow, transitioning to a more subtle and extended halo. There is a slight ellipticity to the overall shape, but it's nearly round.

Color gradients suggest a population of older stars dominating the central region, resulting in a yellowish appearance, while the outer regions may contain younger, bluer stars, or dust. No distinct spiral arms or bar features are discernible. There is no obvious sign of recent or ongoing major merger activity; however, minor disturbances could be present but are difficult to discern at this resolution.
