The galaxy presents as a lenticular or edge-on spiral structure, exhibiting a moderate redshift. Its central bulge appears prominent and yellowish, likely indicating an older stellar population. The disk is elongated, appearing significantly longer than it is wide, viewed nearly edge-on. Evidence suggests a relatively smooth morphology with limited indications of major disturbances or ongoing mergers. Star formation appears moderate within the galaxy, although the bulk of activity seems concentrated towards the center. The estimated mass of the galaxy places it within the range of a standard spiral, with no obvious signs of active galactic nuclei based on visual inspection of the image.
