The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is notably elongated, exhibiting an elliptical morphology rather than a clear spiral structure. The light distribution suggests a bulge-dominated system, with a gradual decrease in surface brightness moving outward from the central region. There is no apparent organized disk structure or spiral arm features visible. A slight asymmetry may indicate a minor gravitational interaction. The galaxy exhibits a color gradient from blue in the center to redder hues at the periphery, which may indicate a transition in stellar populations, with relatively younger stars in the core. The galaxy's overall color suggests intermediate star formation activity.
