The galaxy appears as a single, concentrated object with a smooth, round morphology. It exhibits a predominantly yellow-orange hue, suggesting a population of older stars. There is no discernible spiral arm structure or evidence of a prominent disk. The light profile appears relatively uniform, with no indication of bright knots of star formation. There are no signs of recent merger activity or significant tidal disturbances, such as tails or plumes. The overall color and smoothness are indicative of an elliptical galaxy with a substantial stellar mass and suppressed star formation. The galaxy is of moderate size, and possesses a centrally concentrated brightness.
