The galaxy presents as a single, relatively concentrated object, elliptical in shape, with an intermediate roundness. It appears to possess a generally smooth texture, with a slight asymmetry in its light distribution. The color gradient transitions from a core exhibiting yellowish hues to outer regions that exhibit a redder tint, indicating a population of older stars. There is no evidence of spiral arms, a central bar, or a prominent disk. The overall morphology suggests a galaxy that has undergone substantial evolution, potentially due to a merger history that may have smoothed out previous structures. There is no obvious major disturbance occurring at this time.
