The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a yellowish hue, suggesting an older stellar population. A subtle, extended halo with a reddish tinge surrounds the central concentration, potentially indicating the presence of dust or older stars at the periphery. There are subtle hints of asymmetry in the outer regions, though the dominant feature is its elliptical, centrally concentrated structure. The overall light distribution is relatively smooth, suggesting a lack of prominent spiral arms or other distinct morphological features. The object's color indices suggest moderate amounts of ongoing star formation, likely concentrated in the disk region.