The galaxy presents an elliptical morphology, appearing elongated with a smooth light distribution. The central region exhibits a bright, concentrated core, suggesting a high stellar density. Progressing outwards from the core, the galaxy displays a gradual decrease in luminosity. The color profile suggests a population of older stars, indicated by the reddish-yellow hue. There's a subtle indication of a possible disturbance or interaction, manifesting as a slight asymmetry in the outer regions. No clear spiral arm structures are visible. Overall, the galaxy appears to be a relatively quiescent system, with limited ongoing star formation.
