This galaxy exhibits a distinct, elongated morphology. The primary structure presents as a smooth, centrally concentrated bulge exhibiting a yellowish hue suggesting an older stellar population. A flattened disk is observed, oriented nearly edge-on relative to our line of sight. The disk displays a bluer color, indicative of ongoing star formation. There is minimal evidence of significant spiral arm structure. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There might be a minor disturbance on the left side of the galaxy. The overall impression is of a galaxy with a dominant spheroid and a moderately active disk.
