This galaxy presents as a roughly elliptical, disk-like structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Progressing outward, the galaxy displays a transition to bluer tones in its disk, indicative of more recent star formation. There appears to be a minor disturbance to the structure, as the image portrays what appears to be asymmetric regions of light, suggesting a possible tidal interaction. The image portrays an estimated Petrosian half-light radius of approximately 6.7 kpc, indicating a galaxy of substantial size. Its absolute magnitudes suggest it is a luminous galaxy. The star formation rate is moderately active.
