The galaxy exhibits a generally elliptical morphology. Its central region is characterized by a concentrated, bright luminosity, suggesting a significant stellar population density. The light distribution appears smooth, with a gradual decrease in surface brightness from the center towards the outer regions. The galaxy appears moderately flattened, with a ratio of minor to major axis of approximately 0.67. The overall color profile is relatively uniform, with a slight bluer tint. The disk indicates low levels of on-going star formation. No prominent spiral arm structures are visible, suggesting that the system is likely a transition galaxy with an intermediate Sersic index of around 1.10. Overall, the galaxy presents as a relatively quiescent, though still active, system.
