The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light is dominated by a yellowish-orange hue, suggesting an older stellar population and relatively low star formation rate. The galaxy appears elliptical or spheroidal in shape, exhibiting a high degree of roundness. There is no discernible spiral arm structure or distinct dust lanes. The object shows no strong evidence of recent or ongoing major mergers, although a minor disturbance is possible. The overall impression is of a quiescent galaxy with minimal ongoing star formation.
