This galaxy presents as a spiral type, with an inclination that suggests it is close to edge-on from our vantage point. The disk is clearly visible and exhibits loose spiral arms, although their definition is somewhat blurred, possibly due to distance or dust obscuration. The bulge appears moderately sized and concentrated, displaying a yellow-red hue indicative of an older stellar population. There is a noticeable blue tint along the edges of the disk, suggesting ongoing star formation activity within the spiral arms. No obvious bar structure is apparent. There are no clear signs of major mergers or significant disturbances, although there are some hints of minor asymmetry in the disk. Overall, this appears to be a relatively undisturbed spiral galaxy undergoing moderate star formation.
