The galaxy presents as a somewhat elliptical, lenticular structure. The light distribution appears smooth, lacking significant spiral arm features. A central bulge is evident, exhibiting a redder hue compared to the outer regions of the disk. This suggests an older stellar population concentrated towards the galactic center. The outer regions display a bluer color, hinting at the presence of younger, hotter stars, although star formation activity appears relatively subdued across the galaxy. The object's overall shape appears to be somewhere in between round and cigar shaped. There does not appear to be any major disturbances such as tidal tails or multiple nuclei, suggesting that it is not undergoing major merging activity.
