The galaxy presents a somewhat smooth, elliptical appearance, showing a concentrated central bulge. The color gradient transitions from a yellowish-white core to a slightly reddish halo or outer region, indicative of older stellar populations. There is a lack of distinct spiral arm structures, instead displaying a diffuse morphology. The galaxy exhibits a moderate degree of roundness, not appearing highly elongated or disc-like. There is no strong evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity, although subtle asymmetries or minor disturbances may be present upon closer inspection. Based on its color and morphology, this galaxy likely has a relatively low rate of star formation.
