The galaxy presents a somewhat smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outward into a fainter halo. The color profile is relatively uniform, with a subtle shift towards redder hues in the outer regions compared to the bluer core. While a disk-like structure is not prominently visible, there are subtle indications of internal structure or possibly minor disturbances in the outer regions. There is no obvious spiral arm structure or active star forming regions. The galaxy's overall appearance suggests an older stellar population. It is likely a relatively quiescent galaxy with a low star formation rate.
