The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellow-orange hue, indicative of an older stellar population dominating the central region. Surrounding the core, there is a more diffuse, fainter halo or envelope, with subtle color variations suggesting a possible mix of stellar populations. The overall round shape and lack of prominent spiral arms or other distinct features aligns with characteristics of an early-type galaxy. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the image, though there are some very minor disturbances, which could be attributed to a recent or ongoing minor interaction.
