The galaxy presents as a single, dominant object, appearing largely smooth and elliptical in form. It exhibits a concentrated central bulge that gradually diffuses into a less defined halo. The color profile shows a bias towards redder hues, particularly concentrated in the core, suggesting a population of older stars. Hints of bluer regions may indicate some ongoing, albeit subdued, star formation. Overall, there is no evidence of a spiral structure or a significant disk. There is the slightest hint of interaction with a smaller galaxy.
