The galaxy presents as a single, dominant object with an elliptical morphology, exhibiting a smooth, featureless appearance. It shows a well-defined, centrally concentrated core region that gradually diminishes in intensity outwards. The color profile suggests a primarily older stellar population. The overall shape appears mostly round with a very slight elongation. There is no apparent indication of active star formation, spiral arm structures, or major merger events. A subtle, minor perturbation is observed in the galaxy's halo, which could be a dust lane or tidal tail. There is no clearly visible dust absorption or scattering.
