The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall form appears mostly rounded, though there may be slight deviations from perfect circularity. The galaxy exhibits a yellowish hue, indicative of an older stellar population dominating the light output. There is a lack of distinct spiral arms or prominent dust lanes, and no clear evidence of a recent major merger event. The galaxy's appearance suggests a quiescent state with a low star formation rate.
