This galaxy appears to be a spiral galaxy, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish color, which may indicate an older stellar population. The bulge appears relatively symmetrical and rounded. A flattened disk extends outwards from the bulge, displaying a bluer hue suggestive of ongoing star formation, although distinct spiral arms are not clearly resolved. The galaxy exhibits an overall smooth appearance, with no obvious signs of major mergers or tidal disturbances, though some minor disturbances cannot be ruled out. Dust lanes are faintly visible along the plane of the disk, obscuring some of the light from stars behind them. Overall, the galaxy presents a moderate level of star formation activity, with a mass likely around 10^9 to 10^10 solar masses.
