This galaxy presents as an elliptical morphology, with a smooth, diffuse appearance. The color is primarily a yellow-red hue, suggesting an older stellar population with a lower rate of recent star formation. The galaxy exhibits a relatively high degree of central concentration, with the light intensity decreasing gradually from the core outwards. There is no apparent disk or spiral arm structure. The object appears relatively isolated, lacking any obvious signs of tidal interactions or recent mergers. Based on the overall characteristics, it is consistent with being a mature elliptical galaxy.
