The galaxy presents as a somewhat diffuse object, exhibiting a centrally concentrated luminosity profile. While the resolution is limited, the core appears relatively smooth, transitioning to a fainter, more indistinct outer region. There is some evidence of faint features or possibly irregular structures, which may indicate minor disturbances. Overall, the galaxy appears generally elliptical. A redshift value of 0.032022 suggests it is located at a considerable distance. The galaxy’s relatively low SFR (star formation rate) and high SSFR (specific star formation rate) may indicate that most star formation has ended, or is winding down.
