The galaxy presents as a centrally concentrated object with a generally smooth appearance, suggestive of an elliptical morphology. There is no clear evidence of spiral arm structure or a prominent disk component in this image. The central region exhibits a yellowish hue, possibly indicating an older stellar population or the presence of dust obscuration. The outer regions appear slightly bluer, which could be attributed to a younger stellar population. The galaxy shows a slight elongation with an apparent deviation from a perfectly circular shape. There is no obvious sign of tidal tails, strong gravitational lensing, or other indications of recent major merger events. The overall structure points towards a quiescent galaxy, potentially one that has largely ceased significant star formation in the recent past.
