The galaxy presents as a relatively smooth, elliptical or lenticular structure with minimal discernible features. The light distribution suggests a centrally concentrated mass, with a gradual decrease in luminosity outward from the core. Its overall shape is close to round, showing minimal elongation or asymmetry. The color appears predominantly yellow, indicative of an older stellar population with a relatively low rate of star formation. There's no readily apparent spiral arm structure or major dust lane obscuration. No signs of ongoing major merger events or significant tidal disturbances are observed in this image. The galaxy appears as an isolated object with a regular, well-defined morphology.
