This galaxy presents as a spiral galaxy viewed at a moderate angle, not quite edge-on but also not quite face-on. The disk component is clearly visible. There's evidence of spiral arm structure, which appears somewhat flocculent and not tightly wound. A central bulge is also noticeable. The bulge has a yellowish color, potentially indicating an older stellar population. Some regions within the disk show bluer colors, which suggests ongoing star formation. There is also one noticeable, redder, bright spot on one side of the galaxy, potentially indicating HII regions or dust obscuration. The overall morphology suggests an intermediate-type spiral galaxy, possibly with a bar structure. The galaxy does not present with obvious signs of a major merger event, but minor disturbances might be present.
