The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth overall texture, suggesting it is likely an elliptical galaxy. The central region displays a concentrated, brighter yellowish-white hue, potentially indicating an older stellar population. Progressing outward from the core, the color gradually shifts to a reddish-orange tone. There appears to be minimal evidence of distinct spiral arms or substantial dust lanes. The galaxy does not seem to be undergoing any major merger events. A minor disturbance could be present, though no distinct tidal tails or other major distortions are clearly visible. The galaxy has an estimated diameter of around 5.7 kpc.
