The galaxy appears as a slightly elongated, diffuse object. A central bulge is visible, exhibiting a smooth, concentrated light profile, suggesting a relatively high stellar density in that region. The color of the bulge appears subtly redder compared to the outer regions. Surrounding the bulge is a fainter, less concentrated disk, which seems to be oriented somewhat edge-on relative to our line of sight. The outer regions of the disk fade gradually into the background, indicating a less active star-forming environment at the periphery. There is no clear evidence of spiral arm structure or significant dust lanes within the visible portion of the galaxy. The overall appearance points to a morphological type somewhere between elliptical and lenticular, with a relatively smooth and evolved stellar population. There is no strong evidence of any recent or ongoing major merger events, or strong tidal disturbances in the image.
