The galaxy appears to be a relatively smooth, single object, exhibiting a centrally concentrated light profile. The overall shape seems to be somewhat elliptical, leaning towards round. There is a suggestion of a slight color gradient, with a hint of bluer hues on the periphery and tending towards redder, warmer tones towards the central region. There is no obvious disk component or spiral arm structure visible. There is no clear evidence of any major mergers or strong tidal disturbances in this image, suggesting a relatively settled morphology. There is no single, highly luminous core, and no clear evidence of ongoing, extremely high star formation. Overall, the light distribution suggests a fairly evolved system.
