The galaxy presents as a single, well-defined object, exhibiting a smooth, largely featureless morphology with an elliptical appearance. Its overall color profile suggests a dominant population of older stars, based on the redder hues observed. There is a slight concentration of light toward the center, indicative of a central bulge, but it does not appear to be exceptionally pronounced. There is no visible disk structure or prominent spiral arms. The overall shape is notably rounded with an absence of major disturbances, hinting at a relaxed system that has likely undergone minimal recent merger activity. While there may be a minor asymmetry or possible tidal feature visible, it does not appear to significantly affect the overall smooth, well-defined shape of the galaxy.
