The galaxy presents a largely smooth, elliptical morphology. The dominant central region appears nearly spherical with a high degree of circular symmetry. The galaxy exhibits a radial luminosity profile, brightest at the core, fading gradually outwards. The galaxy color is generally yellowish suggesting an older stellar population. There is no strong evidence of spiral arm structure or prominent dust lanes. The lack of sharp features and the smooth appearance suggests a relatively evolved system. The lack of strong blue colors indicates low ongoing star formation. The galaxy appears isolated, with no significant tidal distortions or nearby companions obviously interacting, suggesting it has undergone no major merging events in recent times.
