The galaxy presents as an elongated, lenticular shape, strongly suggesting an edge-on disk galaxy. It appears relatively smooth in texture, with a brighter central bulge that fades gradually into the outer disk. The central bulge exhibits an ovoid profile. The galaxy does not display any obvious spiral arm structures or prominent dust lanes that might indicate recent major merger activity. The color gradient suggests a slightly redder core, potentially indicative of an older stellar population, transitioning to a slightly bluer hue in the outer disk which is suggestive of younger stars or ongoing star formation. There is no evidence of a significant tidal disturbance or interaction with other galaxies nearby. Based on the high likelihood of the galaxy being viewed edge-on, it is difficult to assess the true morphological type in detail.
