The galaxy presents a centrally concentrated, generally smooth morphology. The core exhibits a bright, yellowish hue, indicative of an older stellar population and potential dust presence. Moving outward from the core, the galaxy displays a more diffuse and slightly bluer halo, suggesting ongoing or recent star formation activity at the outer edges. No distinct spiral arm structures or bar features are readily apparent. Overall the galaxy appears to be fairly round in shape with some minor disturbances visible in its structure.
