The galaxy presents a largely smooth morphology. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. The surrounding disk appears more bluish, potentially indicating ongoing star formation. The galaxy is approximately round in shape. There are some hints of disturbances in the disk region, although no significant ongoing merger events are directly visible. It does not have a distinct cigar shape. Overall, the galaxy appears to be a relatively massive system, exhibiting both characteristics of an elliptical and a spiral galaxy.
