The observed galaxy appears to be an elliptical galaxy with a generally smooth morphology. The galaxy exhibits a moderate level of roundness, with a slight deviation from a perfectly circular shape. The overall color profile suggests a population of older stars, indicated by the reddish-yellow hue, indicating minimal recent star formation. There is no apparent spiral structure or a well-defined disk component in the galaxy, implying a classification towards early-type galaxies. The image suggests a high likelihood of no major disturbances due to mergers or interactions, suggesting a relatively isolated system.
