The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration with a bright, yellowish core. The light appears to gradually decrease in intensity moving outward from the center towards its undefined edges. There is very faint evidence of what may be a dust lane or other feature residing on the upper edge of the galaxy, though the resolution prevents positive confirmation. The absence of distinct spiral arm structures suggests a galaxy type earlier in the Hubble sequence, potentially an elliptical galaxy. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances.
