The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape approximates a flattened spheroid, with the longest axis roughly twice the length of its shortest axis. The light distribution suggests a dominant bulge component, with a smooth transition to a faint, extended halo. The color profile transitions from yellow-white in the central region to a more greenish hue in the outer regions. There is no evidence of spiral arm structure or dust lanes. The morphology indicates a relatively evolved galaxy, possibly an elliptical or lenticular type, with minimal ongoing star formation activity. There are no obvious signs of recent mergers or tidal disturbances.
