The object appears to be a spiral galaxy, viewed nearly edge-on from our vantage point. A prominent central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component shows a bluer color, potentially indicative of ongoing star formation. The disk itself is relatively smooth in appearance, showing little to no evidence of strong spiral arm structures or major dust lanes. There might be some minor disturbances within the disk, but no significant merger activity or tidal features are apparent. The bulge morphology seems rounded. The absence of sharp features in the disk could imply that the galaxy is relatively evolved.
