The galaxy presents as a relatively smooth, elongated structure. It exhibits a color gradient, with a central region displaying a yellowish-orange hue, potentially indicative of an older stellar population or dust obscuration. The outer edges of the galaxy show a faint bluish tint, suggestive of ongoing star formation in these regions. There is a subtle extension, or possible tidal feature, visible at one end of the major axis, hinting at a possible past interaction or minor disturbance. Overall, the galaxy appears to be an early-type spiral or lenticular galaxy, viewed at an angle, with some evidence of recent or ongoing star formation.
