The galaxy presents as a moderately luminous, elliptical structure. The light is concentrated towards the center, with the intensity gradually diminishing outwards. The overall color appears to be redder in hue, suggesting an older stellar population with reduced active star formation. The morphology seems generally smooth, with no apparent spiral arm structures or significant dust lanes. The galaxy's shape is somewhat elongated, leaning towards an intermediate elliptical classification. There is no clear evidence of ongoing mergers or major disturbances to the overall structure.
