The galaxy exhibits an overall elliptical morphology. Its color profile displays a yellowish-orange hue in the central region, suggesting an older stellar population. The outer regions appear fainter and slightly bluer, indicating the presence of some younger stars or potential dust lanes, though the resolution limits a definitive identification. The galaxy's shape is somewhere between round and elongated; there is evidence of some distortion. There is asymmetry in the disk. There appears to be a minor disturbance or interaction possibly a merging event, based on slight irregularities in the outer regions.
