The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. Its light profile exhibits a concentrated central region that gradually diffuses outwards. The core region has a bright, yellowish-white hue, suggesting a population of older stars. Surrounding this central bulge is a fainter, somewhat bluer halo or extended disk. The blueish tint could indicate the presence of younger stars, or ongoing star formation within that region, although the overall smoothness suggests a relatively quiescent system. There is no strong evidence of spiral arms or significant dust lanes. The galaxy appears well-defined but slightly elongated, indicating a possible deviation from perfect sphericity. Overall, this galaxy seems to be a relatively evolved system.
