The galaxy presents a generally smooth, elliptical morphology with no obvious spiral arm structures or distinct features such as bars or rings visible in the image. The light distribution suggests a high degree of central concentration, with the brightest region appearing nearly circular and gradually fading towards the outer edges. The colour profile is dominated by yellow and red wavelengths, indicative of an older stellar population and a relatively low rate of on-going star formation. There is no evidence of any major mergers or significant tidal disturbances in its immediate vicinity, although a slight asymmetry or minor perturbation in the outer halo might be present. The galaxy does not seem to be highly elongated.
