The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated core. The overall color suggests a population of older stars, particularly within the bulge, which is a yellow hue. There is very little evidence of spiral arms or dust lanes. The galaxy appears to be a relatively relaxed system, with no strong signs of ongoing major mergers or significant tidal disturbances. The overall shape appears somewhat elongated, but not markedly so. There may be a faint, extended halo surrounding the main body of the galaxy, indicated by a gradual fading of light intensity outwards from the center, however this is difficult to assess precisely. The overall structure suggests an evolved system.
