The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth luminosity profile. Its color index suggests the presence of an older stellar population. The galaxy's overall form is close to round, with subtle deviation, but not a clear spiral disk. No major disturbances or tidal features are visible, indicating a lack of recent major merger activity. The light profile doesn't show evidence of spiral arms or a well-defined bar. It appears to be in a relatively quiescent state, consistent with a system where star formation is occurring slowly.
