The galaxy presents as a moderately luminous, disk-shaped system, exhibiting a slightly inclined orientation relative to our line of sight. The central bulge appears significant, characterized by a concentrated, yellowish-white hue, suggesting an older stellar population. Moving outward from the bulge, the disk displays a mottled texture with a blend of blue and subtle reddish tones, potentially indicative of ongoing star formation regions intermixed with more evolved stellar populations. The disk's spiral structure appears relatively disorganized. There are no indications of significant tidal disturbances or ongoing major mergers within the visible structure of this galaxy. Overall the galaxy appears relatively undisturbed, though some minor disturbances cannot be ruled out. The outer regions of the disk gradually fade into the background sky, making a precise determination of its full extent challenging.
