The galaxy presents as a moderately bright, elliptical-like structure, displaying a relatively smooth overall morphology with hints of a disk. It exhibits a slightly elongated shape, leaning toward a cigar-like appearance. The galaxy's central region appears brighter and more concentrated than its outer regions. We see a color gradient from red to blue, indicating there may be ongoing or recently ceased star forming regions. No signs of any major mergers are visible, although some minor disturbances cannot be ruled out. Overall, the galaxy seems to be in a stable or near-stable state.
