The galaxy exhibits an elliptical morphology, with a smooth, centralized distribution of light. The color profile suggests a higher concentration of older stellar populations in the core, indicated by the yellowish hue. The light distribution transitions gradually from the central bulge outwards, showing no distinct spiral arm structures or prominent dust lanes. The overall shape appears slightly elongated, but not extremely so. There may be some evidence of minor tidal disturbances but none of the arms or halos are sharp. The galaxy appears to be a fairly massive system. It's star formation rate appears to be low.
