The galaxy presents a largely smooth morphology. It appears elliptical in shape, significantly elongated with a high degree of axial ratio. The light profile exhibits a concentration toward the center, suggesting a prominent bulge. The color appears generally reddish and yellowish, with the central bulge tending more towards the yellow end of the spectrum. There is a hint of fainter, bluer light in the outer regions, suggesting some level of star formation is present, but the object appears to be comprised primarily of older stellar populations. There is no evidence of spiral arms or a distinct disk structure, and no signs of a major ongoing merger, though subtle asymmetric features cannot be entirely ruled out. The galaxy is estimated to be quite massive with a low specific star formation rate.
