The galaxy presents as a centrally concentrated, relatively smooth, and slightly elongated object. Its color profile indicates a higher concentration of light in the redder wavelengths, with some contribution from green. This suggests a population dominated by older stars. There is little to no evidence of significant star formation activity across the galactic disc. Based on the available data, this galaxy is estimated to be of considerable mass. It appears to be largely undisturbed, showing no strong indication of recent or ongoing merger events.
