The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. There is a high concentration of light towards the center, suggesting a prominent bulge. The overall shape is somewhat elongated, deviating slightly from a perfect sphere. The color profile indicates a population of older stars, with a yellowish-red hue dominating the galaxy's light output. There is no visible dust or active star formation regions. Based on the image, there appears to be some potential distortion in the main body and the presence of a close companion to the left side of the object, suggestive of a potential ongoing interaction or merger event. A fainter object can be seen below the galaxy, but its relationship is uncertain from this image. The galaxy has a calculated mass placing it as a very large object with a relatively low rate of star formation.
