The galaxy presents as a lenticular or early-type spiral galaxy at a redshift of approximately 0.095, corresponding to a distance where its projected size is several kiloparsecs. The morphology is largely smooth with some indications of a disk structure. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluish disk, indicative of more recent star formation, although the rate of star formation appears to be low. There is no prominent bar structure visible, and any spiral arms are faint and tightly wound. The overall shape of the galaxy is elliptical, with an axial ratio indicating it is significantly flattened. There are no obvious signs of ongoing major mergers or tidal disturbances. The color gradients suggest a radial variation in stellar populations, with older, redder stars concentrated in the bulge, and younger, bluer stars in the disk.
