The galaxy presents as a centrally concentrated object with a generally smooth profile, though subtle irregularities can be observed. A dominant, yellowish central bulge or core region is visible. The isophotes appear elongated, suggesting an elliptical morphology, or possibly a disk galaxy viewed at an angle. Fainter, bluish-tinged regions are present on one side of the galaxy extending away from the core, potentially indicating areas of ongoing star formation. The overall color index suggests a population of older stars is more prominent throughout, with the potential for a more recent, but less extensive, burst of star formation in a localized area. There is no apparent spiral structure, but there may be some tidal features or faint plumes present. The object doesn't seem to be undergoing any major merger event but shows signs of minor disturbance.
