The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The overall color profile suggests a relatively older stellar population, with a dominant yellow-orange hue. The isophotes appear regular, without significant distortions or tidal features indicating recent major merger activity. However, subtle irregularities along the outer edges might suggest minor disturbances or ongoing accretion events. The galaxy's elongated shape indicates a degree of rotational support, though not as pronounced as in a spiral galaxy. There is no apparent evidence of a distinct disk component or spiral arms. The galaxy appears relatively quiescent in terms of star formation, consistent with its reddish color and smooth morphology.
