The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates the overall luminosity. The color appears to be generally redder, suggesting an older stellar population within the galaxy. The isophotes seem relatively regular, indicating a relaxed dynamical state. There are no obvious spiral arms or significant dust lanes visible in this image. Faint, diffuse extensions are present, hinting at a possible halo structure surrounding the main body of the galaxy. There is minimal evidence of ongoing star formation activity based on the color and lack of bright blue regions. There may be a very slight asymmetry but overall it shows little distortion, indicating no major recent interaction or merger.
