The galaxy presents as an elliptical morphology, appearing elongated with a high degree of axial ratio. The light distribution appears smooth and centrally concentrated, suggesting a lack of significant star formation in the recent past. The color profile indicates an older stellar population, with redder hues dominating the central region. No spiral arms or dust lanes are clearly discernible. The galaxy does not exhibit signs of any major ongoing merger activity, though minor irregularities in its outer isophotes cannot be ruled out at this resolution.
