The galaxy presents as a relatively smooth, centrally concentrated object with an overall elliptical morphology. The light distribution suggests a dominant spheroid component. There is a slight elongation visible, but the galaxy appears largely rounded. There is a possible hint of a feature suggestive of a disk or spiral arm structure within the galaxy, however, the resolution does not allow for a confident assertion. The color profile exhibits a general trend from a somewhat bluer hue in the inner region to redder colors towards the outer edges. This suggests a declining population of young, hot stars towards the periphery, with a possible gradient in star formation activity. There is a hint of some minor disturbance within the galaxy that could potentially indicate an ongoing or past interaction with another galaxy.
