The galaxy presents as a relatively smooth, elliptical object. It exhibits a central concentration of light, appearing brightest in the inner regions and gradually fading towards the outer edges. The core exhibits a subtle reddish hue, possibly indicative of an older stellar population or dust obscuration. The galaxy appears slightly elongated, with an intermediate ellipticity. There may be very faint, diffuse hints of a disk-like structure. The galaxy exhibits a weak blue tint in the periphery, potentially indicating a small amount of more recent star formation. There are no obvious signs of spiral arms or a distinct bar. The galaxy appears isolated, with no clear evidence of ongoing mergers or major tidal disturbances, though subtle disturbances can't be ruled out. Overall, the galaxy presents as a evolved system, likely a massive galaxy with moderate star formation occurring.
