This galaxy exhibits a clear disk-like morphology, observed edge-on from our vantage point. The central bulge region appears relatively prominent, displaying a yellowish-orange hue, potentially indicative of an older stellar population. The disk appears elongated, with a bluish tint towards the outer edges. The presence of blue suggests ongoing star formation in these regions. The galaxy appears relatively smooth, with little indication of spiral arm structures due to its edge-on orientation. There is also no clear sign of a major merger or significant tidal disturbances. The disk shows slight asymmetry. This could be due to the distribution of dust, recent star formation or a minor interaction.
