The galaxy appears to be a disk galaxy, presenting an edge-on orientation relative to our line of sight. The overall form is lenticular, with a smooth, extended profile. A central bulge is not clearly discernible, but the slight increase in surface brightness near the center suggests its presence. The galaxy exhibits a fairly uniform color distribution across its visible extent. There is no evidence of prominent spiral arms or significant dust lanes from this view. It appears relatively undisturbed, lacking signs of major mergers or tidal interactions. The color suggests a mixture of stellar populations.
