The galaxy presents as a luminous, centrally concentrated object with a primarily smooth morphology. It appears to be elliptical or lenticular in shape, with a high degree of roundness. There is minimal evidence of spiral arm structure or distinct disk features. The galaxy exhibits a color gradient, with a yellowish core suggesting an older stellar population, potentially dominated by red giants. The outer regions display a slightly bluer hue indicating the presence of some younger stars, though this is not very prominent. The galaxy appears isolated, without any major signs of ongoing merger activity or significant tidal disturbances. Minor irregularities in its outer regions might indicate past interactions, or perhaps be caused by background/foreground light sources. Overall, the galaxy appears relatively quiescent.