This galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. It exhibits a gradual decrease in luminosity from its bright core outwards, with no distinct spiral arm structures or prominent dust lanes visible. The color gradient suggests a relatively older stellar population. There appears to be a faint, extended halo surrounding the main body of the galaxy, fading into the background sky. There's a slight elongation in the shape, hinting that it may be considered an in-between shape. No obvious signs of major mergers or tidal disturbances are apparent upon visual inspection. The integrated light suggests modest star formation activity is occurring.
