The galaxy appears to be a relatively smooth, elliptical or lenticular type. It is somewhat rounded in shape, though not perfectly circular, with a slight elongation. There is a bright, concentrated central bulge that dominates the galaxy's luminosity profile, indicating a high stellar density in the core. The color is generally reddish, suggesting an older stellar population with fewer young, hot stars. There is little evidence of prominent spiral arms or dust lanes; the overall structure lacks significant distinguishing features. The outer regions of the galaxy gradually fade into the background sky, with no sharp edges indicating a clear boundary. No strong tidal features or signs of major recent mergers are immediately visible. There might be very minor asymmetries or disturbances.
