The galaxy presents an overall elliptical morphology. It appears moderately luminous, exhibiting a diffuse, extended halo surrounding a brighter, more concentrated central region. The color gradient suggests a redder core transitioning to bluer outer regions. This could be indicative of an older stellar population in the center, with younger, bluer stars populating the spiral arms or outer disk. There is a hint of possible faint spiral arm structure, although it is not well-defined. There may be some evidence of minor disturbances in the outer regions of the galaxy, possibly due to interactions with smaller galaxies. Based on its color and morphology, the galaxy likely has a significant stellar mass and a moderate rate of star formation.
