The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears largely uniform, fading gradually towards the outer edges. The core exhibits a yellowish-white hue, suggestive of an older stellar population. A subtle bluish halo surrounds the core, potentially indicating the presence of younger, hotter stars or ongoing star formation within the outer regions. There appears to be a slight, subtle disturbance within the main body. No distinct spiral arms or significant dust lanes are visible in the image. The galaxy's overall morphology suggests it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy.
