The galaxy appears to be a relatively smooth, elliptical type, exhibiting a high degree of central concentration. Its overall shape is approximately round. There is little evidence of distinct spiral arms or a well-defined disk structure. The galaxy displays a color gradient, with the central region appearing more yellow, indicating an older stellar population. Fainter, bluer light can be seen in the outer regions which suggests areas of younger stars. There are hints of minor disturbances, possibly caused by a small merger event. Based on its color and morphology, this galaxy is consistent with an early-type galaxy undergoing passive evolution.
