The galaxy presents a somewhat diffuse, elliptical morphology, appearing relatively smooth with only subtle internal features discernible. A central, brighter region is visible, suggestive of a galactic nucleus or a region of increased stellar density. Fainter, extended emissions surround this core, exhibiting a slight elongation indicative of a flattened spheroidal shape rather than a perfectly spherical one. The color profile seems largely uniform, with faint blue hues permeating the galaxy's structure, but with no high resolution it is difficult to say with certainty. There is no clear evidence of spiral arms or prominent dust lanes, reinforcing the classification of a smooth, likely evolved system. Subtle distortions in the outer regions might indicate past interactions or mergers, although the present image resolution limits the ability to confirm such events without additional spectral and morphological analyses.
