The galaxy presents as a largely smooth, centrally concentrated object with a roughly circular morphology. There is a strong central bulge that exhibits a yellowish hue, suggesting an older stellar population is dominant in that region. Surrounding the core is a more diffuse, bluish halo that appears smoother than the core. This halo might indicate the presence of younger stars, but the lack of distinct spiral arm structures or prominent star-forming regions suggests that star formation activity is relatively low overall. There may be some tidal disturbances present, but it is difficult to see. The galaxy's color profile indicates relatively consistent absolute magnitudes in g, r and z bands. This galaxy likely has a notable stellar mass.
