The galaxy presents an elliptical morphology, appearing relatively smooth and lacking prominent spiral arm structures. Its color profile suggests a population dominated by older stars, exhibiting a yellowish hue. The galaxy displays a moderate degree of roundness. There is no evidence of ongoing major merging activity or significant tidal disturbances in this image, suggesting it is relatively isolated. The rate of star formation appears to be relatively low. Overall, the galaxy appears to be a relatively massive system nearing quiescence.
