The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely elliptical in shape, exhibiting a high degree of rotational symmetry. The central region presents a bright, unresolved core, possibly indicating a supermassive black hole or a dense stellar population. The light distribution decreases smoothly from the core outwards.

There is a subtle colour gradient, the central region appears white/blue with a very slight gradient towards a redder hue as one moves to the outer regions of the galaxy. A slight asymmetry and fuzziness in the outer regions suggests the presence of some minor disturbances, possibly the result of past minor mergers or tidal interactions. There is no clear spiral arm structure visible, with no strong evidence of active star formation. The galaxy is neither undergoing any major merging event nor major disturbances.
