This galaxy presents a largely smooth and concentrated appearance, suggesting characteristics consistent with an elliptical galaxy. It exhibits a centrally concentrated bulge that diminishes in intensity towards its outer regions. Its color profile is slightly redder at the core, indicative of a population of older stars. There is little visible evidence of spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system with a low star formation rate. The shape appears to be somewhat elongated but not highly flattened. Based on the image, there is no apparent interaction with nearby galaxies, indicating that it has been evolving in relative isolation.