This galaxy exhibits a disk-like morphology, appearing largely edge-on from our vantage point. A prominent central bulge is visible, displaying a yellowish hue, suggesting a population of older, redder stars. The disk component shows a bluer color, indicative of younger, hotter stars and possibly ongoing star formation regions. There is a slight hint of dust lanes obscuring parts of the disk, though they do not appear very pronounced. The overall structure appears relatively undisturbed, without obvious signs of a major merger or significant tidal interactions.
