The galaxy presents an elliptical morphology, appearing elongated in shape. The central region exhibits a concentration of light, suggesting a bulge component dominated by older stellar populations, indicated by its reddish hue. Surrounding the bulge, a fainter, more diffuse disk is visible, displaying a greenish tint, potentially signifying the presence of younger, star-forming regions. The disk appears relatively smooth, with minimal evidence of prominent spiral arm structures. Overall, the galaxy appears to be relatively isolated, without any obvious signs of tidal interactions or ongoing mergers, though there is some minor structural disturbance. The red shift indicates it is a moderately distant galaxy.
