The galaxy presents as a centrally concentrated object with a relatively smooth overall morphology. It exhibits a flattened, disk-like structure when viewed from our vantage point. The central region displays a bright, yellowish hue suggestive of an older stellar population. Fainter, bluer colors are present in the surrounding disk, which may indicate more recent star formation activity. There appear to be subtle asymmetries or possible minor disturbances in the outer regions, but no clear signs of major merging activity are apparent. The galaxy appears to be somewhat between round and cigar shaped.
