The galaxy presents as a relatively smooth, disk-shaped structure, exhibiting a pronounced elongation. The primary color is a yellowish-orange hue, concentrated towards the central region, suggesting an older stellar population and/or significant dust obscuration. Fainter, bluish extensions appear at the edges of the disk, possibly indicating regions of more recent star formation. There is a very slight asymmetry in the outer regions of the galaxy suggesting some minor gravitational interaction, although there are no obvious tidal tails or other large-scale disturbances. Based on the observed color and morphology, this galaxy likely falls somewhere between a late-type spiral and an early-type lenticular galaxy.
