The galaxy presents as a somewhat smooth, disk-like structure. While the central region appears more concentrated and brighter, there's a noticeable lack of strong spiral arm definition. The overall color profile suggests a mixture of stellar populations; a bluer hue in the general disk region could indicate ongoing star formation, while the central region seems to display slightly redder tones, possibly associated with older stellar populations. Irregularities are seen, with some disturbances or merging activity potentially present. One side shows evidence of a more significant perturbation. The galaxy is relatively faint, hinting that this is not the most active galaxy in the sky.
