The galaxy presents an elliptical morphology, characterized by a relatively smooth light distribution, and a high degree of central concentration. Its light profile suggests a spheroid-dominated system, with limited or no discernible spiral arm structure. The galaxy's color index is approximately redder in the central regions, becoming subtly bluer towards the outskirts. There is a slight but noticeable elongation in the observed shape, deviating somewhat from a perfect spherical form. No obvious signs of ongoing major mergers or significant tidal disturbances are apparent in the galaxy's morphology. There is some irregular light distribution.
