The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. Its shape appears generally round, with minimal elongation or distortion evident. The color profile indicates a relatively evolved stellar population, with a yellow-white central region. The outer regions exhibit a bluer hue, suggesting the presence of some younger stars. There are no apparent spiral arms, bars, or dust lanes visible. The overall structure suggests a galaxy with a quiescent star formation rate, with most star formation occurring within the central regions. It shows no signs of significant tidal disturbances, suggesting it is not currently undergoing a major merger event.
