The galaxy appears to be a relatively smooth, elliptical system. It presents as a centrally concentrated luminosity profile, with the brightest region located at the core. The overall shape is nearly circular but has a slight tendency to be elongated. While there is no obvious indication of spiral arms or a distinct disk structure, a subtle, low-contrast, disk-like feature might be present. There is no obvious major disturbance or ongoing merging activity, although close inspection reveals possibly slight features which are not easily distinguishable. The galaxy is composed mostly of what is probably older stellar populations, with some recent star formation. This is indicated by the generally yellowish color of the galaxy. Overall, the galaxy seems to be in a relatively relaxed state.
