The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness. There is no strong evidence of spiral arm structures or a prominent disk. The light profile suggests a dominant bulge component.

The central region displays a bright, yellow-white hue, indicating a population of older stars. The outer regions show a gradual fading in intensity, with a slightly redder color suggesting the presence of a cooler stellar population compared to the galactic core. There is no apparent ongoing major merger activity or tidal disturbance based on visible distortions or extended features. However, subtle irregularities in the outer regions cannot be ruled out at this resolution.
