The galaxy presents as a largely smooth, elliptical form, with a high degree of central concentration. The primary light component is bluish in hue, indicative of some ongoing star formation, or a population of relatively young stars, though the rate of star formation is likely low. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat cigar-shaped. There is no visual evidence of significant spiral arm structure or dust lanes. The galaxy appears relatively isolated, with no immediately apparent signs of major tidal interactions or ongoing mergers. However, subtle irregularities in the outer regions may suggest a minor past interaction or disturbance. The color gradients across the galaxy appear minimal, indicating a relatively uniform stellar population throughout the visible extent.
