The galaxy presents a generally smooth morphology. The light distribution suggests an elliptical shape, though possibly with some slight elongation. A central bulge is prominent, exhibiting a yellowish hue, which may be indicative of an older stellar population. There is minimal evidence of strong spiral arm structures or significant star formation regions from the image. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. The color gradient suggests a potential red sequence galaxy, consistent with a more evolved system.
