The galaxy presents as a concentrated elliptical morphology. Its overall structure appears smooth with no visible spiral arms or significant dust lanes. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the central region. The galaxy's color appears to subtly shift towards redder wavelengths away from the core, further supporting an aging stellar population. The overall shape is nearly round, with only a slight deviation towards elongation. There's no strong evidence of recent or ongoing major merger activity, though a minor disturbance cannot be ruled out at this resolution. The galaxy displays a relatively compact structure with no extended halo easily discernible in the image. The relatively small size and redder colors suggests that the galaxy is fairly passive, with a low rate of star formation.
