The galaxy presents as a relatively smooth, concentrated elliptical or lenticular system. The central region exhibits a yellowish-white color, suggestive of an older stellar population and minimal ongoing star formation. The outer regions transition to a slightly redder hue, which could indicate either an aging stellar population, dust obscuration, or a subtle radial color gradient. Overall it is rather smooth in texture. There's no apparent disk structure, spiral arms, or significant morphological disturbance to suggest major interactions. There is a red area that may be a small region of active star formation. The galaxy appears to be quite massive.
