The galaxy presents as a smooth, elliptical object with a high degree of central concentration. The light distribution exhibits a gradual decrease in intensity from the core outwards. There is a distinct absence of spiral arms or prominent dust lanes. The galaxy has a pronounced cigar-like shape with an axial ratio that suggests a classification towards the E4-E6 range on the Hubble sequence. The core region appears yellowish-white, indicating an older stellar population. The lack of blue light signifies low ongoing star formation within the galaxy. There is no evidence of any major mergers or tidal disturbances. The galaxy shows no signs of interactions with other galaxies nearby.
