The galaxy presents as a prominent disk galaxy, viewed nearly edge-on from our vantage point. There is an apparent central bulge, bright and somewhat concentrated, with a yellowish-orange hue suggesting a population of older stars. The disk exhibits a bluer color, indicating the presence of younger, hotter stars and possibly ongoing star formation. The disk appears relatively smooth, without any immediately obvious spiral arm structure or distinct dust lanes. The overall shape is elongated, consistent with an edge-on orientation. No signs of major mergers or significant tidal disturbances are readily apparent.
