The galaxy presents as an elongated, ellipsoidal structure, indicative of a possible elliptical or lenticular morphology. The light distribution appears relatively smooth, with a central concentration that gradually decreases towards the edges. There is a hint of a disk-like structure, but no clear spiral arms or bar features are visible. The galaxy displays a reddish hue, suggesting an older stellar population with lower ongoing star formation. There is no evidence of major mergers or tidal disturbances. Subtle hints of a minor disturbance cannot be ruled out but would need further investigation. The overall impression is a galaxy in a relatively quiescent state of evolution. The galaxy is likely a massive object with a low specific star formation rate.
