This galaxy appears to be a relatively smooth, disk-dominated system. Its overall shape is elongated, suggesting a possible edge-on orientation relative to our line of sight. A central bulge is visible, exhibiting a yellowish hue, potentially indicative of an older stellar population. The disk component shows a bluer color, hinting at the presence of younger, hotter stars and ongoing star formation, though at a low rate. There is no evidence of major mergers or strong tidal disturbances. Minor asymmetries within the disk are not ruled out. Based on its size, this galaxy is likely a massive system.
