The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. It is observed as a nearly circular object, indicative of a minimal inclination relative to our line of sight. Color gradients appear subtle, with a suggestion of redder hues towards the core region and slightly bluer tints in the outer regions, though overall the color is relatively uniform. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy seems to be relatively isolated, with no visually obvious signs of ongoing mergers or tidal disturbances. Some minor asymmetries are visible, but they do not appear to represent a major interaction. Overall, the galaxy appears to be a quiescent, early-type system.
