The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, bright core, potentially indicating a supermassive black hole actively accreting material. The light distribution suggests a radial falloff in surface brightness from the core outwards, characteristic of an elliptical morphology. The galaxy lacks any distinct spiral arm features or prominent dust lanes.

The overall color appears to be yellowish-white, suggestive of an older stellar population dominated by evolved stars. A subtle blueish halo surrounds the central region, hinting at the presence of some younger, bluer stars, although the overall star formation rate seems to be low. The smooth, round morphology and color profile align with properties expected for an elliptical galaxy at a moderate redshift, which would explain its moderate luminosity. No apparent signs of ongoing major mergers or tidal disturbances are observed, indicating a relatively undisturbed evolutionary history for this system.
