The galaxy appears as an elongated, disk-shaped structure with a noticeable central bulge. The core region exhibits a bright, yellowish hue, suggesting a concentration of older stars. Proceeding outwards from the center, there's a transition to a reddish color, hinting at the presence of dust lanes and potentially ongoing star formation, though it is not immediately obvious in the image. The disk appears relatively smooth overall, without prominent spiral arm features. There is a subtle warp in the galaxy's disk, and a hint of a possible tidal tail or distortion on one side, which could indicate a past or ongoing interaction with another galaxy, though not a major merger. The galaxy does have some signs of disturbance in the outskirts. Based on the colors, it may be undergoing relatively low levels of star formation.
