The galaxy appears to be a relatively compact and luminous object, exhibiting a centrally concentrated light profile. Its morphology suggests a significant spheroidal component, likely a large bulge or elliptical shape. The color distribution is not uniform; a yellowish hue dominates the central region, potentially indicative of an older stellar population. Fainter, bluer components extend outwards from the core, possibly representing younger star formation regions within a disk or extended halo. There are hints of some faint disturbances, but overall the galaxy presents as a singular object with a relatively smooth appearance. 
