The galaxy presents as an elliptical morphology, exhibiting a smooth and somewhat spheroidal appearance. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. There is a color gradient visible, with a redder hue towards the center and a bluer tint in the outer regions. The galaxy's disk is either not present or it's being viewed edge on, thus obscuring any spiral arm structures. Subtle disturbances may be present, indicating possible past gravitational interactions, but no clear major merging events are visible. The overall structure suggests a relatively evolved galaxy with ongoing, albeit potentially moderate, star formation activity.
