The galaxy presents a relatively smooth, elliptical morphology, exhibiting a bright, concentrated central bulge that dominates its overall structure. The light distribution appears centrally concentrated with the galaxy's luminosity decreasing gradually from the core to the outer regions. There is a very slight elongation along a major axis, but it appears nearly circular. The color is generally yellowish-orange. There is no obvious presence of spiral arms or dust lanes, suggesting an older stellar population. There may be an apparent lack of ongoing, or recent, star formation activity. The galaxy shows minimal signs of tidal distortions or interactions, indicative of a relatively isolated evolutionary history.
