The galaxy presents as a somewhat elliptical structure with a high degree of central concentration. The light is relatively smooth with no prominent spiral arm features visible. The major axis of the ellipse is notably longer than the minor axis, though it does not exhibit an extremely elongated, cigar-like shape. Color gradients suggest a relatively uniform stellar population, trending slightly redder towards the central bulge. Overall the system has an old stellar population with limited ongoing star formation. There are no obvious signs of interaction or recent merger events, though minor disturbances cannot be entirely ruled out.
