This galaxy exhibits a primarily smooth morphology. It appears somewhat elongated in shape, with an aspect ratio that suggests it is neither perfectly round nor highly flattened. There is a distinct central bulge that is relatively bright and concentrated. The color of the central bulge appears yellowish, possibly indicating an older stellar population. Fainter, bluer light extends outward from the bulge, hinting at the presence of a disk component with ongoing star formation. There is no strong evidence of a prominent spiral structure or major disturbances. The galaxy appears to be relatively isolated, with no immediate signs of ongoing or recent major merger activity. Overall, this galaxy presents as a relatively evolved system, possibly a lenticular galaxy or an elliptical galaxy with some residual star formation.
