The galaxy appears as a single, centrally concentrated object with a smooth light distribution. The galaxy's color is a relatively uniform yellowish-white hue, suggesting a dominant population of older stars. The object presents as moderately round, exhibiting a subtle deviation from perfect circularity, tending towards a slightly elliptical shape. There is no obvious dust lane or spiral structure. The galaxy does not appear to be undergoing any major merger events, nor are there any apparent tidal tails or other signs of strong gravitational disturbance.
