The galaxy presents a generally smooth morphology, appearing largely featureless in this imaging. It exhibits an elliptical shape, appearing mostly round. The light profile is centrally concentrated with a bright core, which gradually fades into a more diffuse outer region. The galaxy's overall color appears yellowish-red, suggesting an older stellar population and potentially lower rates of ongoing star formation. No obvious spiral arms or dust lanes are discernible. There is no evidence of major mergers or significant tidal disturbances. Minor disturbances may be present based on subtle asymmetries or irregularities in the galaxy's outer regions, but require higher resolution imaging for confirmation.
