The galaxy presents as a centrally concentrated, largely featureless object. Its overall shape appears elliptical, with a smooth, diffuse light profile. The core region is brighter and more compact. The galaxy has a slightly bluish hue near its center, possibly indicating the presence of younger, hotter stars in the region. The outer regions are redder, which may signify an older stellar population or the presence of dust. There is no evidence of a distinct spiral structure or a prominent disk. No ongoing major merger events are clearly visible, but a minor interaction cannot be ruled out based on the available image data. Overall, the galaxy appears to be a relatively evolved system with a somewhat suppressed star formation rate.
