The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, featureless morphology with a high degree of central concentration. It appears largely spheroidal, with an apparent circularity, showing minimal deviation from a rounded shape. There is no obvious spiral arm structure or bar feature visible. The galaxy's color profile is consistent with an older stellar population; it displays a redder hue. There are no signs of ongoing major merging activity or significant tidal disturbances. The galaxy is likely a relatively massive system, exhibiting substantial luminosity. Overall, it is indicative of a galaxy that has largely completed the process of hierarchical structure formation and is undergoing passive evolution.
