The galaxy appears to be a spiral galaxy, oriented approximately face-on with a slight tilt. Two prominent spiral arms emanate from the central bulge, exhibiting a moderately open winding pattern. The arms show some patchiness, suggestive of localized star formation regions. A strong central bar-like feature is visible bisecting the bulge. The bulge itself appears moderately sized relative to the disk. There is no visual evidence of a major ongoing merger, but there might be minor disturbances in the outer regions of the disk. The color distribution indicates a relatively normal spiral galaxy, with a yellowish central bulge and bluer spiral arms, indicative of a mix of older stellar populations in the bulge and younger, hotter stars within the arms. The overall structure is well-defined, suggesting a relatively undisturbed system.
