The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits a flattened, ellipsoidal shape, tending towards a slightly elongated form rather than perfectly circular. The light distribution suggests a dominant spheroidal component, characteristic of an elliptical galaxy or the bulge of a spiral galaxy. The color gradient transitions from a bright, yellowish-orange core to a fainter, redder halo. This color suggests an older stellar population within the galactic bulge, with a possible contribution from dust reddening in the outer regions. Evidence of any spiral arm structure or distinct star-forming regions is absent, indicating either a lack of ongoing star formation or obscuration by dust. It seems to have undergone no major recent merger events, suggesting a dynamically relaxed state.
