The galaxy appears as a relatively smooth, elliptical structure with a prominent central bulge. The color gradient suggests a population of older stars, with a yellowish-orange hue dominating the central regions. Fainter, bluer light can be seen extending from the central bulge along the equatorial plane of the galaxy, suggesting some regions of more recent, albeit low, star formation. The galaxy shows an elongated morphology. There are no obvious signs of spiral arm structures or major disturbances indicative of ongoing mergers. There might be a faint disk component, but it is not well-defined. The galaxy presents as isolated and quiescent.
