The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. A distinct, yellowish central bulge is visible, suggesting a concentration of older stellar populations. Surrounding the bulge, a more diffuse, bluish halo extends outwards. This halo likely contains a population of younger, hotter stars, and possibly ongoing star formation. The galaxy appears generally rounded in shape, with no obvious spiral arm structures or other prominent features indicative of a disk galaxy. There are subtle irregularities in the outer halo, which could indicate minor disturbances or interactions, but the galaxy does not appear to be undergoing a major merger or exhibiting strong tidal features. Overall, the galaxy presents a relatively quiescent and well-mixed appearance.
