The galaxy exhibits an elliptical morphology, appearing largely smooth with a high degree of central concentration. It's shape is neither perfectly round nor elongated, rather it appears somewhat in between these two extremes. The central region presents a yellowish hue, suggesting a population of older stars. Fainter, bluer extensions are visible emanating from the core of the galaxy, indicative of some more recent, but mild, star formation activity in these areas. No strong spiral arm structure or significant dust lanes are discernible. There are some small features visible surrounding the galaxy that appear to be disturbances, suggesting a minor merger event may have occurred.
