The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, though it appears somewhat intermediate in shape, with only a slight elongation. The galaxy's color profile suggests a population of older stars, exhibiting a reddish hue overall. There is no apparent spiral structure. A bright central bulge is clearly visible, with a gradual decrease in light intensity outwards, suggesting a centrally dense distribution of stars. The edges of the galaxy fade gradually into the background, showing no sharp truncation. There is some indication of a minor disturbance, suggesting the possibility of an interaction or merger history. There is no indication of intense star formation.
