The galaxy presents a generally smooth morphology, exhibiting a central concentration of light that gradually decreases outwards. There is a noticeable color gradient, shifting from a more yellow-ish hue in the core to bluer tones in the outer regions. The shape appears to be elliptical, although the overall roundness is not particularly pronounced. No spiral arm structures are discernible. There is no evidence of a major merger or tidal disturbances. The galaxy seems to have a moderate to high mass and a moderate amount of star formation.
