The galaxy presents as a spiral structure with a prominent, moderately sized central bulge. The spiral arms are well-defined, exhibiting a relatively loose winding pattern. Two spiral arms appear to dominate the structure, emanating from the central bulge and extending outwards. The colour of the galaxy suggests a mix of stellar populations; the central bulge displays a yellowish hue, indicative of older, cooler stars, while the spiral arms show bluer regions, implying ongoing star formation. There is no obvious signs of a major ongoing merger or significant tidal distortion. The image suggests a generally undisturbed, relatively evolved spiral galaxy.
