The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated bulge of light that fades gradually towards its periphery. Its overall shape is elongated, appearing somewhat cigar-shaped. The core region is a bright, yellowish hue, which may indicate an older stellar population dominating the central region. The smooth light distribution suggests a relatively homogenous stellar population. The galaxy shows no signs of prominent disk features or spiral arms, and the overall texture appears smooth. There is no indication of recent major merger activity; the galaxy presents as a relatively undisturbed, evolved system.
