The galaxy presents a largely smooth, elliptical morphology. The central bulge is dominant and appears uniformly luminous with a bright, concentrated core. The galaxy exhibits a yellowish hue, suggestive of an older stellar population and relatively low current star formation activity. There's a slight elongation observable, but it's largely in between round and elongated, without any clear spiral arm structures or prominent dust lanes. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. The galaxy displays a relatively compact size, but with a significant amount of mass for its size, which is expected given the lack of major features. The faint outer regions suggest a gradual decline in stellar density.
