The galaxy presents a largely smooth and rounded morphology. There is minimal evidence of spiral arms or a prominent disk structure. The galaxy's light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color profile suggests a dominant population of older stars, exhibiting a yellowish to reddish hue, indicative of reduced recent star formation activity. No significant tidal features, mergers, or major disturbances are discernible, suggesting a gravitationally settled system.
