The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. The central bulge appears bright and concentrated, exhibiting a yellowish hue, possibly suggesting an older stellar population. A fainter, extended disk is oriented horizontally, showing a slight bluish tint. A small percentage of the galaxy appears disturbed, indicating a possible past merger event or tidal interaction. The galaxy overall lacks strong spiral arm structures, which suggests a reduced star formation rate.
