The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless structure. Its light profile suggests a high degree of central concentration, with the intensity gradually decreasing outwards. The galaxy appears to be moderately luminous, with a color gradient indicating a redder core, possibly due to an older stellar population. There is little evidence of spiral arms or a distinct disk component. Tidal features and major disturbances are not apparent, indicating that this galaxy is likely in a relatively isolated state, or has undergone only minor interactions in the recent past. The overall shape is best described as "in between", appearing not fully rounded or elongated. Its apparent lack of distinct features suggests a quiescent system. 
