The galaxy presents a largely smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, gradually decreasing in intensity towards the outer regions. The overall color profile appears relatively uniform with a dominant yellow hue, suggesting a population of older stars and a lower rate of ongoing star formation. There is a slight blue tinge towards the very edges of the galaxy. The galaxy's shape is generally round, with no obvious indication of spiral arm structures or significant tidal disturbances. There is no current evidence of a major ongoing merger, though there may be very slight disturbances. The redshift of 0.307851 suggests the galaxy is at a considerable distance. Given the smooth appearance and the absence of significant features, the galaxy is likely a mature system.
