This galaxy exhibits a smooth, elliptical morphology with a concentrated central bulge. The luminosity profile gradually decreases from the core outwards, displaying no distinct spiral arm structures or prominent star-forming regions. The color distribution suggests a population of older stars, with a redder hue in the central region that transitions to slightly bluer tones towards the periphery. There is no obvious evidence of recent merger activity or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed, indicative of a system that has undergone substantial evolution and potentially possesses a low star formation rate.
