The galaxy presents as a single, relatively smooth light distribution. The light profile appears centrally concentrated, exhibiting a radial decrease in intensity from a bright core. The shape is approximately circular, with a slight elongation perceptible along one axis. There are no distinct features or spiral arms visible; the galaxy appears largely amorphous. Color gradients are subtle, transitioning from a bluer core to redder outer regions. The outer region of the galaxy looks slightly fuzzy but with no obvious visual distortions or tidal features. No indication of ongoing or recent merger events is apparent. Based on the color profile and morphology, the galaxy likely has relatively low levels of star formation.
