The galaxy presents as a relatively smooth, elliptical-like form. It exhibits a prominent central bulge, characterized by a yellowish hue, likely indicating an older stellar population. The light intensity diminishes gradually from the core outwards. There is an apparent disk or flattened component with a slight blue tint. The galaxy displays a moderate elongation, with its shape deviating from a perfect circle. Visual assessment indicates a system that is generally undisturbed, although a very slight irregularity on one side could indicate a past minor interaction. There may be ongoing but low levels of star formation occurring in the outer regions.
