The galaxy presents as an elongated structure, possibly a spiral seen at a high inclination or a lenticular galaxy. A smooth, concentrated central bulge is apparent, displaying a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluish regions extend from either side of the bulge along the major axis, indicating the potential presence of younger, hotter stars and ongoing star formation within what might be spiral arms or a disk component. There appears to be a slight asymmetry in the overall structure, indicating that the galaxy may have experienced a minor gravitational disturbance, though there are no clear signs of major tidal features or an ongoing merger.
