This galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent bulge is visible, concentrated at the galaxy's center, exhibiting a yellowish hue, suggesting an older stellar population. The disk component is elongated and relatively smooth, with a bluish tinge, possibly indicating the presence of younger stars and ongoing star formation, even if subdued. There is no sign of strong disturbances or tidal features in the disk or halo, indicating it's most likely not undergoing a major merger, and is relatively isolated. 
