The galaxy presents as an edge-on spiral, characterized by a prominent, centrally concentrated bulge. The disk component is clearly visible, exhibiting a flattened morphology and appears to be well-defined. The bulge displays a smooth, rounded structure, with a color gradient indicative of an older stellar population. The disk shows variations in color and brightness, possibly indicative of spiral arm structure, though not distinctly resolved. There is a small region near the central bulge that is redder than the rest of the galaxy. The overall shape is elongated, consistent with a high inclination angle relative to our line of sight. There are no clear signs of ongoing major merger events. The galaxy is relatively isolated, with no obvious close companions or tidal features.
