The galaxy presents as a relatively smooth, disk-like structure with a slight elongation. The overall color appears to be trending towards redder wavelengths, suggesting an older stellar population. There is minimal evidence of distinct spiral arms or active star formation regions. A slight asymmetry can be observed in the outer regions of the galaxy, perhaps indicating a minor gravitational disturbance or past interaction. The galaxy seems to be generally isolated in its immediate surroundings, with no readily apparent major companions or signs of an ongoing merger. The galaxy possesses a relatively high mass.
