The galaxy presents as a centrally concentrated object with a generally smooth appearance. There is a slight elongation to the morphology, deviating from a perfectly circular form. The galaxy appears to be dominated by an elliptical profile, with no prominent spiral arms or distinct disk-like features readily discernible in the available image. A color gradient is observed, with a shift towards redder hues in the central region, indicating a potentially older stellar population. Fainter, bluer areas exist around the central, yellow region, suggesting some more recent, but minimal star forming regions. There is no indication of any major ongoing merger activity or strong tidal distortions. Based on the overall appearance, this galaxy is likely a mature system with a significant spheroidal component and subdued star formation.
