The galaxy appears to exhibit a relatively smooth morphology, with a dominant, centrally concentrated spheroid component. The core region is characterized by a distinct yellowish hue, suggestive of an older stellar population or significant dust obscuration. A fainter, bluish extended structure is visible, possibly indicating ongoing star formation in a more diffuse disk or halo. The object presents a slightly elliptical shape, with no prominent spiral arms or bar structures readily apparent. The overall visual impression is that of a relatively evolved system, potentially undergoing or having undergone a recent or ongoing merger event.
