The galaxy exhibits a prominent disk morphology, observed nearly edge-on from our vantage point.  The central bulge appears bright and concentrated, displaying a yellowish hue.  The disk component extends outwards from the bulge, with a bluer color gradient toward the outer edges, suggestive of ongoing star formation within the disk.  The disk appears relatively smooth, without obvious signs of major spiral arm structures.  There are faint, subtle signs of disturbances. The galaxy appears to be relatively isolated, with no obvious signs of recent or ongoing major mergers.
