The galaxy presents as a lenticular or possibly an elliptical galaxy, with a generally smooth, featureless appearance. It displays an elongated, cigar-like shape. The central region appears brighter and more concentrated in luminosity, suggesting a dense galactic nucleus or bulge. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a bluer periphery. This color variation indicates potential differences in stellar populations, with older, redder stars concentrated toward the center and younger, bluer stars potentially populating the outer regions, although the blue component is not distinct. There may be some minor asymmetries or disturbances in the galaxy's outer regions. The galaxy's morphology suggests it has undergone a period of relative quiescence with regards to major merging events recently.
