The galaxy presents as a moderately bright, resolved structure with a notable disk component. The disk appears inclined relative to our line of sight, exhibiting an elongated shape. There is some evidence of spiral arm structure, though it is not sharply defined. The central bulge is prominent and appears relatively smooth and concentrated, with a yellowish-orange hue indicating an older stellar population. The disk exhibits a bluer tint, which is consistent with ongoing star formation. There is an indication of some minor disturbance or possible tidal features around the galaxy, but nothing suggestive of a recent major merger. Overall, the galaxy appears to be a spiral type with intermediate to high stellar mass and an active, but not extreme, rate of star formation.
