The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population dominating the central region. Faint greenish-blue extensions are visible emanating from the central region, possibly indicating regions of more recent, albeit subdued, star formation. The galaxy appears largely undisturbed, showing little evidence of tidal features or major mergers. The overall morphology suggests a galaxy with a significant spheroidal component and potentially a weak disk. The shape appears close to round.
