The galaxy appears to be a spiral galaxy viewed at a slight angle. It presents a central bulge that is bright and yellowish in color, suggesting an older stellar population. A disk component is visible, though not perfectly edge-on. Faint spiral arm structures can be discerned, though they are somewhat diffuse, hinting at moderate star formation activity. There seems to be a slight asymmetry or disturbance in the overall structure, as well as an indication of a possible minor merging event, with some tidal features or an irregular shape. The disk exhibits a bluer tint compared to the bulge, indicating the presence of younger, hotter stars. The galaxy is relatively large, with a considerable extent.
