The galaxy presents as a single, largely featureless object. It exhibits a centrally concentrated luminosity profile, with the peak emission appearing yellowish-white. The overall morphology suggests a system with minimal disk-like features or spiral arm structures. The elliptical shape indicates that the system is not perfectly spherical, showing signs of some slight elongation. The color gradient is smooth, with no obvious regions of intense star formation or dust lanes visible in this observation. The galaxy displays a smooth texture, suggesting an older stellar population. The overall appearance of this galaxy indicates a relatively evolved system which is likely no longer undergoing major star formation. Some level of minor gravitational disturbance cannot be entirely ruled out due to the slight asymmetry in the galaxy's shape, but there are no clear signs of a major ongoing or recent merger event.
