The galaxy appears as a concentrated central bulge, surrounded by a fainter, diffuse disk. The central bulge displays a yellowish-orange hue, potentially indicating an older stellar population. The disk component shows a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. Overall, the galaxy exhibits a relatively smooth morphology, though there is evidence of subtle features or disturbances within the disk. Based on color and morphology, this is likely a spiral or lenticular galaxy undergoing active star formation in its outer regions.
