The galaxy presents as a relatively smooth, elliptical structure, elongated in shape. It is likely a disk galaxy viewed at an angle. A central bulge is apparent, exhibiting a yellowish hue, suggesting an older stellar population. The outer regions display a fainter, bluish tint, which could indicate the presence of younger, hotter stars and ongoing star formation. Overall, the galaxy appears to be in a relatively quiescent state, with no obvious signs of major mergers or tidal disturbances. The morphology suggests a late-type spiral or early-type elliptical galaxy at a moderate redshift.
