The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution with a fairly round morphology. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy displays a color gradient, shifting from a reddish hue in the central region to a more greenish-yellow color in the outer regions. This could indicate the presence of older stellar populations and potential areas of more recent star formation in the outer disk. No major merging or tidal disturbance is apparent, though there is some slight asymmetry which could imply a minor interaction at some point in the galaxy’s history.
