This galaxy exhibits a generally smooth morphology with a distinct cigar shape. There is evidence of a faint disk-like structure with a bulge. The galaxy appears to be relatively isolated, showing no signs of major interactions or mergers, although the data suggests minor disturbances cannot be ruled out. Color gradients indicate a redder core and bluer disk, suggesting ongoing star formation, although its specific star formation rate is relatively low. Overall, the galaxy seems to be an elliptical galaxy with a hint of a disk.
