The galaxy presents as a relatively compact, elliptical object. Its overall color profile suggests a lack of significant recent star formation, with a dominant yellow hue indicating an older stellar population. The light distribution appears smooth and centrally concentrated, showing minimal evidence of spiral arms or prominent disk structures. A slight elongation is noticeable, suggesting a deviation from a perfectly spherical morphology. There might be a subtle indication of a minor tidal disturbance, but it's difficult to discern any major disruption or ongoing merger activity. The galaxy appears to be a quiescent, evolved system with a substantial stellar mass.
