The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape, although it is not perfectly round. The central region displays a bright, yellowish hue, suggestive of an older stellar population and minimal ongoing star formation. Moving outward from the center, the color shifts to a redder tone, possibly indicating a decreasing age of stars or increased dust extinction. There is no obvious spiral structure or distinct disk, but rather a gradual decline in luminosity from the core to the outer regions. The galaxy does not show strong evidence of recent or ongoing mergers, although there appears to be a minor perturbation on the galaxy's right side.
