The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its light profile suggests a relatively uniform stellar population distribution, lacking prominent spiral arms or distinct features. The core of the galaxy displays a higher concentration of luminous material, potentially indicative of an active galactic nucleus or a dense stellar bulge. There is a slight elongation to the shape, but it is mostly round. The color index suggests that it may be an older, more evolved system composed of mainly older stars. There are no apparent signs of recent or ongoing major merger activity. The overall structure is consistent with an early-type galaxy.
