The galaxy presents a largely smooth, elliptical morphology. It appears elongated with a cigar-like shape. The color profile suggests a population of older stars, with a dominant reddish-yellow hue in the central bulge, indicative of lower star formation rates. There is a hint of blue in the outer regions, which may be related to younger star formation. The overall structure indicates it is likely not undergoing any major merging events, although some minor disturbances may be present. The galaxy is estimated to be approximately 4.4 kpc in radius. Its observed redshift indicates that it is at an approximate distance of 433 megaparsecs from the Earth. 
