The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be generally elliptical, though not perfectly spherical; it seems to lean towards being somewhere in between circular and elongated. There is a slight suggestion of a disk-like structure, but it is not strongly pronounced. The central region displays a higher surface brightness, likely indicative of a concentrated galactic nucleus or bulge. There is little evidence of significant ongoing merger activity or major disturbances in its overall structure. The galaxy exhibits a smooth, featureless appearance, with no discernible spiral arms or prominent dust lanes. Its overall color is predominantly a pale, neutral hue, suggestive of an older stellar population and relatively low star formation rate.
