The galaxy presents as a relatively luminous, disk-like structure with a notable central bulge. The disk component exhibits a somewhat smooth texture, suggesting a later-type morphology, potentially a spiral or lenticular galaxy seen at an oblique angle. The galaxy appears elongated, with the major axis significantly exceeding the minor axis. The bulge region is bright and concentrated. The color distribution indicates a more prominent contribution from older stellar populations, particularly in the bulge region, which appears redder. The disk shows subtle color variations, hinting at regions of ongoing or recent star formation within the spiral arms, but they are not very pronounced. There is no strong evidence of major mergers or significant tidal disturbances in this image. Any features that might indicate these, are minor.
