The galaxy presents as a centrally concentrated object with a relatively smooth light distribution. It appears elliptical in shape, with a high degree of central concentration that diminishes towards the outer edges. The core exhibits a more reddish hue. There is evidence of some blue coloring surrounding the redder core, potentially indicative of a younger stellar population. No distinct spiral arm structure is visible; instead the light is diffuse and evenly distributed. There is no clear sign of tidal tails or strong gravitational disturbances in the immediate vicinity, although some minor disturbances cannot be ruled out. Overall, the galaxy gives the visual impression of a galaxy with a mostly older stellar population with some on going star formation.
