The galaxy presents as a relatively smooth, elliptical-like object. Its core region exhibits a high surface brightness, appearing almost unresolved and intensely luminous. The light distribution decreases radially outward, displaying a relatively even gradient. There is a subtle color gradient noticeable, with the core exhibiting a slightly redder hue compared to the outer regions which appear bluer. No distinct spiral arm structures or prominent dust lanes are apparent. The overall symmetry suggests a dynamically relaxed system, indicative of an older stellar population or post-merger scenario. There is no evidence of tidal tails or other strong gravitational disturbances in the immediate vicinity of the galaxy. The morphology aligns with a spheroid-dominated galaxy.
