The galaxy presents an overall smooth morphology, suggesting an elliptical or lenticular classification, although some features or a disk component cannot be entirely ruled out. The main body of the galaxy exhibits a centrally concentrated light distribution, appearing roughly rounded in shape. There is a suggestion of a slight elongation or distortion, but not highly pronounced. The color profile indicates a redder core region transitioning to a bluer halo, hinting at older stellar populations dominating the center, with potential ongoing star formation in the outer regions. Evidence of any major merger events is not strongly apparent, but minor disturbances or interactions cannot be excluded. A notable feature is the presence of a distinct, bright, reddish-orange region offset from the main galactic nucleus, which may indicate an area of concentrated star formation, a tidal dwarf galaxy or a background galaxy that has been gravitationally lensed.
